This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1
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
target,2461148.6113,13.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1113 13.67CV 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
target,2461148.6113,13.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1113 13.89CV 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
ATO J102.1837+01.2286,2461148.6113,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J102.1837+01.2286 20260418.1113 13.60CV 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 3112044006023794304,2461148.6113,13.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112044006023794304 20260418.1113 13.63CV 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
GDS_J0656420-021737,2461148.6113,13.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J0656420-021737 20260418.1113 13.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.2771-02.2334,2461148.6113,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.2771-02.2334 20260418.1113 13.66CV 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 3101884656022743680,2461148.6113,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3101884656022743680 20260418.1113 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6113,13.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1113 13.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.6901-02.2242,2461148.6113,13.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.6901-02.2242 20260418.1113 13.53CV 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
ATO J105.8705-02.3904,2461148.6113,13.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.8705-02.3904 20260418.1113 13.42CV 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
ATO J102.7908-02.3649,2461148.6113,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J102.7908-02.3649 20260418.1113 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108790478098341120,2461148.6113,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108790478098341120 20260418.1113 13.46CV 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 3108860782423215232,2461148.6113,13.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108860782423215232 20260418.1113 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107647265186582528,2461148.6113,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107647265186582528 20260418.1113 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6113,13.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1113 13.39CV 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
ATO J103.8067-00.4589,2461148.6113,13.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.8067-00.4589 20260418.1113 13.55CV 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
ATO J104.6668-01.9250,2461148.6113,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.6668-01.9250 20260418.1113 13.24CV 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
ASASSN-V J064630.95+010809.2,2461148.6113,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J064630.95+010809.2 20260418.1113 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6113,13.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1113 13.42CV 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
ATO J103.4280-01.9828,2461148.6113,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.4280-01.9828 20260418.1113 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.6707-05.7846,2461148.6113,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J101.6707-05.7846 20260418.1113 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112107704678242432,2461148.6113,13.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112107704678242432 20260418.1113 13.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6113,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1113 13.20CV 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
target,2461148.6113,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1113 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6113,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1113 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J100.4699-05.2164,2461148.6113,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J100.4699-05.2164 20260418.1113 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J102.7070-01.3966,2461148.6113,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J102.7070-01.3966 20260418.1113 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3100972989085022976,2461148.6113,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3100972989085022976 20260418.1113 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112469585742136064,2461148.6113,13.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112469585742136064 20260418.1113 13.18CV 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
GDS_J0704359-031646,2461148.6113,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J0704359-031646 20260418.1113 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6113,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1113 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J0703252-030259,2461148.6113,13.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J0703252-030259 20260418.1113 13.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6113,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1113 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6113,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1113 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114569137555198464,2461148.6113,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114569137555198464 20260418.1113 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6113,12.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1113 12.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.9152-04.6412,2461148.6113,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.9152-04.6412 20260418.1113 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106052732803548160,2461148.6113,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3106052732803548160 20260418.1113 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.3525-02.5480,2461148.6113,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.3525-02.5480 20260418.1113 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0385 Mon,2461148.6113,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0385 Mon 20260418.1113 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6113,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1113 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114694099624336256,2461148.6113,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3114694099624336256 20260418.1113 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3105965733946504448,2461148.6113,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3105965733946504448 20260418.1113 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6113,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1113 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109336454339492608,2461148.6113,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109336454339492608 20260418.1113 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3102372667384237952,2461148.6113,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3102372667384237952 20260418.1113 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J098.7797-03.0546,2461148.6113,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J098.7797-03.0546 20260418.1113 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3053304074782543488,2461148.6113,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3053304074782543488 20260418.1113 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.7374-04.6394,2461148.6113,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.7374-04.6394 20260418.1113 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
target,2461148.6113,12.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1113 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
Gaia DR3 3112130214607270656,2461148.6113,12.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112130214607270656 20260418.1113 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 J103.6522-00.6011,2461148.6113,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.6522-00.6011 20260418.1113 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 3101049125963883520,2461148.6113,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3101049125963883520 20260418.1113 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3125504223071142784,2461148.6113,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3125504223071142784 20260418.1113 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112314039208032000,2461148.6113,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112314039208032000 20260418.1113 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3053416980884797824,2461148.6113,12.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3053416980884797824 20260418.1113 12.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J065448.56+002321.1,2461148.6113,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J065448.56+002321.1 20260418.1113 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112424230887731712,2461148.6113,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112424230887731712 20260418.1113 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.6490-04.3421,2461148.6113,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.6490-04.3421 20260418.1113 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3105921684761121152,2461148.6113,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3105921684761121152 20260418.1113 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3105621277567743360,2461148.6113,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3105621277567743360 20260418.1113 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6113,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1113 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.4233-01.3658,2461148.6113,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.4233-01.3658 20260418.1113 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108833221613004800,2461148.6113,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108833221613004800 20260418.1113 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3101515288839155328,2461148.6113,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3101515288839155328 20260418.1113 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3126153111029053568,2461148.6113,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3126153111029053568 20260418.1113 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.0676-03.0161,2461148.6113,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.0676-03.0161 20260418.1113 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.1574+00.2897,2461148.6113,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.1574+00.2897 20260418.1113 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6113,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1113 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112948251257159808,2461148.6113,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112948251257159808 20260418.1113 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3101401729901835904,2461148.6113,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3101401729901835904 20260418.1113 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107281540128223104,2461148.6113,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107281540128223104 20260418.1113 12.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J0651481-040224,2461148.6113,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J0651481-040224 20260418.1113 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3125607134785759744,2461148.6113,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3125607134785759744 20260418.1113 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3105302831513609216,2461148.6113,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3105302831513609216 20260418.1113 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112503842401083904,2461148.6113,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112503842401083904 20260418.1113 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106340014576032512,2461148.6113,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3106340014576032512 20260418.1113 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J102.9043-01.6544,2461148.6113,13.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J102.9043-01.6544 20260418.1113 13.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3125637852391270784,2461148.6113,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3125637852391270784 20260418.1113 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113913996125565440,2461148.6113,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113913996125565440 20260418.1113 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106128697885405184,2461148.6113,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3106128697885405184 20260418.1113 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6113,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1113 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113534462753024768,2461148.6113,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113534462753024768 20260418.1113 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.4580-02.6934,2461148.6113,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.4580-02.6934 20260418.1113 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6113,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1113 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113219246514568576,2461148.6113,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113219246514568576 20260418.1113 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6113,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1113 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6113,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1113 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J102.7477+00.2283,2461148.6113,13.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J102.7477+00.2283 20260418.1113 13.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J099.7145+01.2057,2461148.6113,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J099.7145+01.2057 20260418.1113 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6113,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1113 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108863080225629056,2461148.6113,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108863080225629056 20260418.1113 13.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113700076693885568,2461148.6113,13.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113700076693885568 20260418.1113 13.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112396051604609408,2461148.6113,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112396051604609408 20260418.1113 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113408362514158720,2461148.6113,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3113408362514158720 20260418.1113 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.8055-05.8431,2461148.6113,13.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.8055-05.8431 20260418.1113 13.35CV 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 3119353181365762048,2461148.6113,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3119353181365762048 20260418.1113 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J100.4835+00.2927,2461148.6113,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J100.4835+00.2927 20260418.1113 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112496798656101504,2461148.6113,13.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112496798656101504 20260418.1113 13.35CV 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
ASAS J065055-0458.5,2461148.6113,13.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J065055-0458.5 20260418.1113 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6113,13.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1113 13.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112223325200684160,2461148.6113,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112223325200684160 20260418.1113 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106021564222428032,2461148.6113,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3106021564222428032 20260418.1113 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6113,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1113 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112311565306916096,2461148.6113,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112311565306916096 20260418.1113 13.38CV 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
ATO J103.4491-02.6658,2461148.6113,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.4491-02.6658 20260418.1113 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106181925419346432,2461148.6113,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3106181925419346432 20260418.1113 13.29CV 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
ATO J103.9614-02.2114,2461148.6113,13.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.9614-02.2114 20260418.1113 13.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6113,13.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1113 13.35CV 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
ATO J103.1164-04.3756,2461148.6113,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.1164-04.3756 20260418.1113 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6113,13.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1113 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.9413-02.3695,2461148.6113,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.9413-02.3695 20260418.1113 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3102564188568694912,2461148.6113,13.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3102564188568694912 20260418.1113 13.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J106.8218-02.7605,2461148.6113,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.8218-02.7605 20260418.1113 13.48CV 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
ATO J101.4694-00.5200,2461148.6113,13.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J101.4694-00.5200 20260418.1113 13.63CV 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
target,2461148.6113,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1113 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6113,13.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1113 13.63CV 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
target,2461148.6113,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1113 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6113,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1113 13.60CV 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
target,2461148.6113,13.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1113 13.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.3533-02.2202,2461148.6113,13.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J107.3533-02.2202 20260418.1113 13.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6113,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1113 13.71CV 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 J104.6381-01.6369,2461148.6113,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.6381-01.6369 20260418.1113 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3102935892216786560,2461148.6113,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3102935892216786560 20260418.1113 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6113,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1113 13.60CV 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
target,2461148.6113,13.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1113 13.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.1246+01.9093,2461148.6113,13.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.1246+01.9093 20260418.1113 13.73CV 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
target,2461148.6113,13.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1113 13.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J103.8575+00.6544,2461148.6113,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.8575+00.6544 20260418.1113 13.64CV 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
target,2461148.6113,13.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1113 13.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3105839977303968896,2461148.6113,13.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3105839977303968896 20260418.1113 13.93CV 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 J104.3488-02.6186,2461148.6113,13.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.3488-02.6186 20260418.1113 13.86CV 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 3112415366075378304,2461148.6113,13.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112415366075378304 20260418.1113 13.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461148.6113,13.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1113 13.78CV 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
target,2461148.6113,13.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260418.1113 13.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J102.5168-01.1896,2461148.6113,13.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J102.5168-01.1896 20260418.1113 13.63CV 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
First image: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Last image: 2461148.61160512 18.04.2026 02:40:32.682 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 20
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.85
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: 11 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): 31509
Objects passed selection criteria: 31394
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 25330
Average stars matched: 22941.2 (90.5695 %)
Memory usage VmPeak: 131816 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 Fri Apr 17 22:09:47 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: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
First image: 2461032.81363703 23.12.2025 07:31:28.239 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Last image: 2461148.61160512 18.04.2026 02:40:32.682 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 340
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.50
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: 334 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): 226845
Objects passed selection criteria: 226137
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 185249
Average stars matched: 168585 (91.0047 %)
Memory usage VmPeak: 2021220 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 Fri Apr 17 22:17:28 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits
SExtractor catalog cache: saved Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat to cache
SExtractor catalog cache: saved Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.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/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.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: 2461148.61096332
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits exists and is non-empty
Saving wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits to local_wcs_cache/
'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> 'local_wcs_cache/wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits exists and is non-empty
Saving wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits to local_wcs_cache/
'wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> 'local_wcs_cache/wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits'
wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits (1st reference image)
verification OK: wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Image size: 931.8'x623.6' 15.5(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.84"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:51:43.082 -02:00:16.78 J2000 4789.000 3195.000
###################################
The image scale is 5.84"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits (1st new image)
verification OK: wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits
Image size: 937.2'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:51:19.773 -02:01:29.65 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:19.773 -02:01:29.65
Angular distance between the image centers 0.0991 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits (2nd new image)
verification OK: wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:51:22.722 -02:01:07.53 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:22.722 -02:01:07.53
Angular distance between the image centers 0.0859 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 06:51:19.773 -02:01:29.65
Second-epoch second image center 06:51:22.722 -02:01:07.53
Angular distance between the image centers 0.01373 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/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits &> /tmp/tmp.xv0KeNeCsY
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits &> /tmp/tmp.1Hc9MUnwvs
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits &> /tmp/tmp.ld1t7z7FeF
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits &> /tmp/tmp.rVJSM7U2yW
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits
Calibrating the magnitude scale
Found non-empty wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
Found non-empty wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
The reference image (wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits) and catalog (wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat) found
'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat' -> 'wcsmag.cat'
Read 36622 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 95.0306 to 110.7538 deg, Dec -7.3378 to +3.4896 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 95.0306 to 110.7538 deg, Dec -7.3378 to 3.4896 deg
Loaded 24069 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): 377 out of 430 total matches.
Matched with Tycho-2 430 out of 36622 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.893893
a=0.000000 b=1.000000 c=22.893893
From vast_summary.log: estimated ref. image limiting mag.: -7.85
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.04
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.04
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 19 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.1 pix Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
2.1 pix Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
2.5 pix fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits
2.5 pix fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits
Limiting magnitude estimates:
15.0 mag. Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
15.0 mag. Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
14.7 mag. fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits
14.7 mag. fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 11.8 (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.xv0KeNeCsY (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> 'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS-calibrated image found: wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Checking if the catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS catalog name: wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=4596, passed=36622
Got 36622 stars (including 31982 good ones) from the SExtractor catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
util/solve_plate_with_UCAC5 got 36622 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 931.8'
Seting catalog search parameters based on the expected field of view 931.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012942 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010353 (37.3 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 469 (Dec -7.3 to 3.5)
Done reading UCAC5 zone files...
Matched 457 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 347 matched stars entering correct_measured_positions(), 270 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 10.06"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 338 matched stars entering correct_measured_positions(), 14588 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 16.11"
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 413 to 469 (Dec -7.3 to 3.5)
Done reading UCAC5 zone files...
Matched 489 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 392 matched stars entering correct_measured_positions(), 14615 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 16.01"
Accuracy estimation diagnostic: 390 matched stars entering correct_measured_positions(), 15067 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 12.91"
Excluding outliers - 390 stars left (next iteration limit 371)
The image catalog is written to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits -region wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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.1Hc9MUnwvs (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> 'wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS-calibrated image found: wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Checking if the catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS catalog name: wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=4657, passed=36412
Got 36412 stars (including 31701 good ones) from the SExtractor catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
util/solve_plate_with_UCAC5 got 36412 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 625.6'
Seting catalog search parameters based on the expected field of view 625.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.008689 (31.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.006951 (25.0 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 435 to 488 (Dec -3.0 to 7.4)
Done reading UCAC5 zone files...
Matched 20 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Retrying with a larger catalog search radius.
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 435 to 488 (Dec -3.0 to 7.4)
Done reading UCAC5 zone files...
Matched 73 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 51 matched stars entering correct_measured_positions(), 0 with non-zero local correction accuracy
ERROR: the estimated accuracy of the plate solution seems unrealistically small! No stars (out of 51 matched) have non-zero estimated_local_correction_accuracy.
ERROR running correct_measured_positions()
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.ld1t7z7FeF (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_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.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_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2900, passed=29000
Got 29000 stars (including 26083 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits.cat
util/solve_plate_with_UCAC5 got 29000 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 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 413 to 468 (Dec -7.4 to 3.3)
Done reading UCAC5 zone files...
Matched 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 918 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 28515 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
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 413 to 468 (Dec -7.4 to 3.3)
Done reading UCAC5 zone files...
Matched 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 28513 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 28513 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
Excluding outliers - 929 stars left (next iteration limit 1021)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.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.rVJSM7U2yW (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_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.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_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2891, passed=29028
Got 29028 stars (including 26116 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits.cat
util/solve_plate_with_UCAC5 got 29028 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 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 413 to 468 (Dec -7.4 to 3.3)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 914 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 28561 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.4 to 3.3)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 28560 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 28560 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.74"
Excluding outliers - 927 stars left (next iteration limit 1020)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
Saving fully-calibrated image wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits'
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits'
Preparing the HTML report for the field Mon-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out51879.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out55562.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56903.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57096.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57163.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57252.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57273.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57427.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57681.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57685.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57693.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57766.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out57935.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 2s
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: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51879_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 51879_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:43:22.37 -00:06:14.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.08, MAG_FAINT_SEARCH_LIMIT=13.06)GAIADR2_OUTPUT=# 2.493 3119487832880590464 100.84344321446 -00.10473488405 11.9491 11.1458 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.493#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54406_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 54406_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 07:09:13.61 -02:21:30.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54579_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 54579_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:42:37.26 -03:49:19.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55562_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 55562_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:48:24.43 -00:31:25.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.56, MAG_FAINT_SEARCH_LIMIT=12.54)GAIADR2_OUTPUT=# 1.180 3113209110392080384 102.10191212973 -00.52416580695 11.6927 11.3805 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.180#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56699_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 56699_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:44:47.50 -05:17:45.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56903_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 56903_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:51:09.59 -02:35:42.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.86, MAG_FAINT_SEARCH_LIMIT=12.84)GAIADR2_OUTPUT=# 1.101 3105917355433930880 102.79000853321 -02.59546837364 11.5920 10.8606 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.101#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57096_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 57096_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:49:36.56 -01:22:54.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.91, MAG_FAINT_SEARCH_LIMIT=12.89)GAIADR2_OUTPUT=# 0.408 3107099119975852544 102.40225282149 -01.38158700736 11.9362 11.4820 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.408#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57163_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 57163_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:52:52.96 -02:21:14.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.94, MAG_FAINT_SEARCH_LIMIT=12.92)GAIADR2_OUTPUT=# 0.858 3106021564222428032 103.22062591715 -02.35415158459 12.2269 12.1110 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.858#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57252_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 57252_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:46:23.83 -02:23:37.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.95, MAG_FAINT_SEARCH_LIMIT=12.93)GAIADR2_OUTPUT=# 0.656 3106155498479577600 101.59922268247 -02.39400212671 11.9676 11.5712 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.656#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57273_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 57273_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:57:08.32 -02:29:10.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 1.195 3108979632757074560 104.28462469204 -02.48666262908 12.0874 11.9026 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.195#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57427_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 57427_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:55:01.52 -02:35:09.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.98, MAG_FAINT_SEARCH_LIMIT=12.96)GAIADR2_OUTPUT=# 1.162 3105971880037872256 103.75633707660 -02.58618377942 11.9457 11.4346 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.162#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57603_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 57603_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:42:24.45 -02:50:13.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57667_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 57667_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:40:30.48 -01:04:42.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57681_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 57681_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:47:59.17 -05:10:37.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 1.132 3102142869455465728 101.99635090709 -05.17744509619 11.9915 11.6437 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.132#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57685_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 57685_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:51:02.64 -03:31:07.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 0.845 3102794600674186752 102.76106487506 -03.51908682196 12.0402 11.8470 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.845#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57693_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 57693_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:50:53.12 +01:21:58.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 3.125 3126065214517150080 102.72155493317 +01.36552187352 12.3588 11.9139 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.125#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57766_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 57766_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:46:11.70 +00:43:51.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 2.060 3125564730568304384 101.54882438523 +00.73037694592 11.7300 10.7580 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.060#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57818_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 57818_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:42:23.77 -02:34:16.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57935_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 57935_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:49:12.11 -01:48:15.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 1.134 3106296235967921664 102.30057640666 -01.80459768529 12.0201 11.6413 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.134#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 3s
Prepared the HTML report for the field Mon-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits
SExtractor catalog cache: saved Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat to cache
SExtractor catalog cache: saved Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Creating symlink local_wcs_cache/wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits exists and is non-empty
wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits exists and is non-empty
wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits exists and is non-empty
wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits (1st reference image)
verification OK: wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Image size: 931.8'x623.6' 15.5(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.84"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:51:43.082 -02:00:16.78 J2000 4789.000 3195.000
###################################
The image scale is 5.84"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits (1st new image)
verification OK: wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits
Image size: 937.2'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:51:19.773 -02:01:29.65 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:19.773 -02:01:29.65
Angular distance between the image centers 0.0991 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits (2nd new image)
verification OK: wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:51:22.722 -02:01:07.53 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 06:51:43.082 -02:00:16.78
Second-epoch image center 06:51:22.722 -02:01:07.53
Angular distance between the image centers 0.0859 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 06:51:19.773 -02:01:29.65
Second-epoch second image center 06:51:22.722 -02:01:07.53
Angular distance between the image centers 0.01373 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/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits &> /tmp/tmp.IATnw77ih0
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits &> /tmp/tmp.e6q3XuKzR0
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits &> /tmp/tmp.rcgQLG7DZ2
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits &> /tmp/tmp.A0D7dHaGRj
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits
Calibrating the magnitude scale
Found non-empty wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
Found non-empty wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits and wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
The reference image (wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits) and catalog (wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat) found
'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat' -> 'wcsmag.cat'
Read 254624 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 95.0305 to 110.7571 deg, Dec -7.3394 to +3.4970 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 95.0305 to 110.7571 deg, Dec -7.3394 to 3.4970 deg
Loaded 24089 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): 401 out of 624 total matches.
Matched with Tycho-2 624 out of 254624 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 21.875059
a=0.000000 b=1.000000 c=21.875059
From vast_summary.log: estimated ref. image limiting mag.: -7.50
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.38
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.38
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 289 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
2.0 pix Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
2.3 pix fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits
2.4 pix fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits
Limiting magnitude estimates:
14.4 mag. Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
14.4 mag. Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
14.0 mag. fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits
14.0 mag. fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 13.3 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.IATnw77ih0 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits' -> 'wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS-calibrated image found: wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Checking if the catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
WCS catalog name: wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=59, blended=45640, passed=254565
Got 254565 stars (including 208571 good ones) from the SExtractor catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat
util/solve_plate_with_UCAC5 got 254565 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 931.8'
Seting catalog search parameters based on the expected field of view 931.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012942 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010353 (37.3 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 469 (Dec -7.3 to 3.5)
Done reading UCAC5 zone files...
Matched 468 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 369 matched stars entering correct_measured_positions(), 265 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.77"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 366 matched stars entering correct_measured_positions(), 92781 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.43"
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 413 to 469 (Dec -7.3 to 3.5)
Done reading UCAC5 zone files...
Matched 498 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 431 matched stars entering correct_measured_positions(), 92827 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.42"
Accuracy estimation diagnostic: 428 matched stars entering correct_measured_positions(), 121659 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.79"
Excluding outliers - 428 stars left (next iteration limit 402)
The image catalog is written to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits -region wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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.e6q3XuKzR0 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits 568.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits' -> 'wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS_IMAGE_NAME=wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS-calibrated image found: wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Checking if the catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits alredy exist and is non-empty...
Catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat corresponding to the image wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
WCS catalog name: wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=58, blended=46013, passed=257598
Got 257598 stars (including 211206 good ones) from the SExtractor catalog wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits.cat
util/solve_plate_with_UCAC5 got 257598 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 625.6'
Seting catalog search parameters based on the expected field of view 625.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.008689 (31.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.006951 (25.0 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 435 to 488 (Dec -3.0 to 7.4)
Done reading UCAC5 zone files...
Matched 17 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Retrying with a larger catalog search radius.
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 435 to 488 (Dec -3.0 to 7.4)
Done reading UCAC5 zone files...
Matched 68 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 44 matched stars entering correct_measured_positions(), 0 with non-zero local correction accuracy
ERROR: the estimated accuracy of the plate solution seems unrealistically small! No stars (out of 44 matched) have non-zero estimated_local_correction_accuracy.
ERROR running correct_measured_positions()
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.rcgQLG7DZ2 (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_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.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_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=56, blended=29874, passed=193061
Got 193061 stars (including 162981 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits.cat
util/solve_plate_with_UCAC5 got 193061 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 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 413 to 468 (Dec -7.4 to 3.3)
Done reading UCAC5 zone files...
Matched 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 917 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 189276 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
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 413 to 468 (Dec -7.4 to 3.3)
Done reading UCAC5 zone files...
Matched 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 189279 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 189280 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Excluding outliers - 938 stars left (next iteration limit 1030)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.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.A0D7dHaGRj (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_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.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_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=65, blended=29799, passed=192195
Got 192195 stars (including 162198 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits.cat
util/solve_plate_with_UCAC5 got 192195 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 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 413 to 468 (Dec -7.4 to 3.4)
Done reading UCAC5 zone files...
Matched 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 913 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.64"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 187811 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.4 to 3.4)
Done reading UCAC5 zone files...
Matched 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 187812 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 187811 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Excluding outliers - 929 stars left (next iteration limit 1023)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.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_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.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_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/wcs_Mon-02-Q2b1x1_2025-12-23_01-31-28_20.00sec_-15.00C_LIGHT_0382.fits
Saving fully-calibrated image wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.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_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/wcs_Mon-02-Q2b1x1_2025-12-23_01-32-16_20.00sec_-15.00C_LIGHT_0383.fits
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.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_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-39-37_20.00sec_-4.90C_LIGHT_0032.fits
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.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_2026-04-17_CI_Mon-02-Q2b1x1_215936_TTUQ2b1x1_1109198_R0bF8ab1/wcs_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033.fits
Preparing the HTML report for the field Mon-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_gaiadr2.txt__out283582.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283608.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283657.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283675.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283679.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out283717.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283721.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283724.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283728.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283738.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283793.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out283820.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out318300.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out318472.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out321580.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out322642.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out322812.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out322997.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out323103.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out324236.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out324889.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out325103.dat to exclusion_list_gaiadr2.txt
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Adding exclusion_list_gaiadr2.txt__out325319.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out325346.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out325395.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out325420.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out325463.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out325536.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out325541.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out325567.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out283569.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283575.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283590.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283607.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283609.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out283621.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283630.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283650.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283656.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out283700.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283716.dat to exclusion_list_local.txt
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Adding exclusion_list_local.txt__out283749.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283759.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283774.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283779.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283785.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283792.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283797.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283807.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283839.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283841.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283846.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283852.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283854.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283872.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283880.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283895.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283900.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283901.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283910.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283916.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283928.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283931.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283939.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283941.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283945.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283949.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283953.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283954.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283963.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283964.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283973.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283975.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283991.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out300356.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out303249.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out303615.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out303623.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out304878.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out305301.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out305664.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out306701.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out307217.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out307705.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out309007.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out309341.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out309397.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out309401.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out309437.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out309706.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out309790.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out310028.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out310572.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out311387.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out311414.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out311502.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out311605.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out311874.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out311926.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out312014.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out312179.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out312966.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out312971.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out313223.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out314159.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out314201.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out314345.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out314417.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out315008.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out315121.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out315169.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out315280.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out315752.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316008.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316684.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out317042.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out317251.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out317324.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out318266.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out318439.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out318481.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out318512.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out318708.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out318756.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out319013.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out319015.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out319114.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out319409.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out319603.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out319606.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out319740.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out319893.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out320037.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out320833.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out321994.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out322331.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out322896.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out322917.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out323104.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out323318.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out323576.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out323612.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out323844.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out323982.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out324068.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out324149.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out324319.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out324402.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out324588.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out324726.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out324851.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out324955.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out324975.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out325080.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out325119.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out325369.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out325388.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out325476.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 164s
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: 89s
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Considering the candidate 283569_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 283569_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 283575_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 283575_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 283577_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 283577_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
Rejecting candidate due to large distance (15.6") between the two second-epoch detections
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Considering the candidate 283582_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 283582_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 07:00:40.53 -02:18:49.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 1.535 3108953450636596992 105.16856807003 -02.31396275987 14.7554 13.9014 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.535#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283590_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 283590_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 283600_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 283600_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 07:02:39.52 -06:05:09.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 283607_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 283607_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 283608_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 283608_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:43:36.85 -00:02:05.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 1.966 3119490070564086784 100.90343429227 -00.03525772612 13.9800 12.9196 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.966#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283609_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 283609_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 283617_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 283617_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 283621_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 283621_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 283630_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 283630_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 283650_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 283650_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 283656_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 283656_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 283657_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 283657_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:59:06.96 +00:37:15.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 3.209 3113816968524447488 104.77868045215 +00.62002909308 14.6083 14.0335 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.209#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283675_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 283675_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 07:09:38.94 -05:20:53.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 3.428 3053350593562904192 107.41133635163 -05.34833743190 14.2498 13.3294 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.428#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283677_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 283677_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 283679_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 283679_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:53:09.17 -04:52:17.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 2.646 3102027867410986368 103.28774393973 -04.87204327137 14.4515 13.9567 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.646#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283685_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 283685_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 283690_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 283690_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 283700_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 283700_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 283701_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 283701_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:59:51.21 -05:11:54.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 1.454 3101581706207520000 104.96334624563 -05.19879181154 14.2698 13.8601 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.454#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283716_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 283716_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 283717_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 283717_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 07:09:15.37 -06:10:47.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 3.797 3053091010044502784 107.31349768652 -06.18071092120 14.2195 13.4911 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.797#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283721_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 283721_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:46:11.71 +00:50:14.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 1.806 3125567891665421568 101.54879744084 +00.83672062076 14.3349 13.7505 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.806#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283723_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 283723_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 283724_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 283724_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:47:23.67 +01:30:18.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 2.685 3125765567538996864 101.84829729096 +01.50441327626 14.1440 13.7368 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.685#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283725_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 283725_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 283728_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 283728_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 07:01:55.53 -06:11:59.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.25, MAG_FAINT_SEARCH_LIMIT=14.23)GAIADR2_OUTPUT=# 1.335 3052869698970583168 105.48124573053 -06.20015329687 14.1228 13.5426 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.335#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283737_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 283737_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 283738_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 283738_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:50:48.83 +00:23:54.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 3.956 3113562912617709440 102.70303164580 +00.39751525708 14.0885 13.0975 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.956#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283740_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 283740_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 283744_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 283744_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 283749_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 283749_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 283751_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 283751_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:42:02.02 +02:11:58.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 283752_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 283752_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:46:14.68 -05:48:19.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 283759_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 283759_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 283774_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 283774_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 283779_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 283779_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 283785_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 283785_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 283792_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 283792_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 283793_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 283793_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 07:00:19.67 -03:32:02.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 2.387 3102620607258624000 105.08153655364 -03.53454019159 13.9178 13.2849 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.387#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283794_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 283794_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:59:20.20 -01:39:38.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 4.317 3112130764363047808 104.83484613740 -01.66162703516 13.9818 13.4656 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.317#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283797_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 283797_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 283807_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 283807_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 283820_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 283820_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 07:01:51.90 +01:20:07.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 2.751 3115367211199527296 105.46601850960 +01.33474391831 14.0347 13.4996 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.751#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283824_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 283824_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 07:09:13.15 -05:36:09.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 2.655 3053335720102368512 107.30444242285 -05.60331698859 13.8254 13.2979 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.655#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283825_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 283825_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 07:08:17.16 -04:56:01.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 2.427 3059427667355169920 107.07112402067 -04.93442171047 14.0267 13.6990 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.427#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283826_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 283826_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:42:17.82 +02:11:06.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 2.394 3126792202162858240 100.57392687056 +02.18444643850 13.9378 13.4510 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.394#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283836_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 283836_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 07:03:25.05 +01:44:08.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 283839_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 283839_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 283841_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 283841_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 283846_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 283846_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 283852_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 283852_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 283854_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 283854_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 283861_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 283861_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:53:48.56 -03:18:59.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 1.756 3102817832155590400 103.45189812196 -03.31686080716 13.6976 12.7865 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.756#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283869_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 283869_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:38:37.49 -02:21:17.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 3.559 3106690204730551936 099.65602265592 -02.35585984284 13.2484 12.1574 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.559#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283872_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 283872_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 283880_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 283880_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283884_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 283884_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:54:26.64 -02:18:18.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 2.124 3105995729997787136 103.61075390990 -02.30575843373 13.8993 12.8680 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.124#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283886_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 283886_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:46:49.11 -00:40:04.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 2.496 3107388433273217536 101.70428377390 -00.66846482585 13.8561 13.4047 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.496#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283888_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 283888_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 07:05:27.57 -01:00:10.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.92, MAG_FAINT_SEARCH_LIMIT=13.90)GAIADR2_OUTPUT=# 1.455 3109568623093291648 106.36453423089 -01.00305075955 13.7684 12.8340 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.455#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283895_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 283895_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 283897_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 283897_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:52:04.45 -05:53:12.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 1.901 3101108259073557760 103.01829861414 -05.88727505251 13.5348 13.0509 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.901#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283900_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 283900_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 283901_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 283901_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 283907_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 283907_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:49:20.28 +01:36:08.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 3.069 3126133285461258240 102.33394828471 +01.60168323993 13.7464 12.9199 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.069#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283910_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 283910_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 283916_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 283916_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283928_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 283928_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283929_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 283929_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 07:08:43.57 +01:59:20.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.67, MAG_FAINT_SEARCH_LIMIT=13.65)GAIADR2_OUTPUT=# 2.368 3114730628324738432 107.18117361815 +01.98960102822 13.4946 12.6526 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.368#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283931_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 283931_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 283935_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 283935_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 07:05:19.36 -01:29:13.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 3.354 3109468056438096000 106.33034015352 -01.48790042039 13.5034 12.6642 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.354#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283939_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 283939_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283941_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 283941_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283943_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 283943_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:46:13.93 +00:50:43.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 3.391 3125567926025169792 101.55788835134 +00.84443176757 13.6372 12.9682 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.391#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283945_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 283945_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283946_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 283946_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:55:05.01 -01:02:55.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)GAIADR2_OUTPUT=# 1.960 3112333899136721408 103.77089108376 -01.04932192669 13.4551 12.7464 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.960#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283949_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 283949_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283953_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 283953_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283954_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 283954_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283955_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 283955_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:57:53.35 -00:24:37.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.42, MAG_FAINT_SEARCH_LIMIT=13.40)GAIADR2_OUTPUT=# 3.066 3112475323818314752 104.47188036842 -00.41113470113 13.3040 12.4449 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.066#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283956_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 283956_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:58:25.52 -02:40:32.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 2.524 3108912390749031168 104.60594672572 -02.67627969568 13.3638 13.0142 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.524#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283958_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 283958_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:46:12.68 +00:51:08.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283963_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 283963_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283964_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 283964_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283966_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 283966_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:57:27.84 -01:45:23.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 2.895 3112044139160625024 104.36522484805 -01.75663240647 13.3959 12.7743 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.895#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283973_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 283973_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283975_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 283975_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283984_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 283984_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:51:02.43 +01:07:15.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283989_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 283989_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:50:49.67 -01:13:39.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.89, MAG_FAINT_SEARCH_LIMIT=12.87)GAIADR2_OUTPUT=# 1.079 3112361520063852800 102.70670591074 -01.22782858409 12.8359 12.4507 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.079#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283991_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 283991_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283994_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 283994_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:56:14.01 -05:00:25.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283998_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 283998_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 07:08:35.64 +01:46:44.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284000_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 284000_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:58:26.63 -00:54:52.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284002_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 284002_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:53:11.76 -01:33:37.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284003_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 284003_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 07:08:38.08 -05:29:36.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 286739_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 286739_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:50:40.18 -00:32:22.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288367_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 288367_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:51:37.24 +00:26:59.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288989_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 288989_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:51:39.75 +00:25:32.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290259_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 290259_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:40:30.58 -01:04:43.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290621_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 290621_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:40:37.74 +00:43:02.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291072_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 291072_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 07:04:10.68 -03:14:37.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291849_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 291849_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:50:41.62 -00:33:42.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 299597_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 299597_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:45:00.21 -00:03:31.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 300000_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 300000_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 07:04:34.86 -05:56:30.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 300033_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 300033_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:45:04.83 -01:02:23.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 2.601 3107346681891637888 101.26967865935 -01.04031808691 13.2059 12.6723 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.601#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 300356_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 300356_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 301027_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 301027_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:38:54.29 +00:00:12.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 2.304 3119634652045900032 099.72581188348 +00.00294192467 13.1884 12.6963 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.304#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 301285_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 301285_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:34:15.07 -05:19:04.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 3.000 3103462897582381312 098.56209663853 -05.31829740534 13.0894 12.5053 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.000#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 302495_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 302495_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:59:52.89 -04:47:26.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 2.222 3101629122646359040 104.96985275355 -04.79110958798 13.3251 12.7714 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.222#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 302543_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 302543_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:43:50.43 +01:35:51.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 303249_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 303249_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 303615_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 303615_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 303623_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 303623_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 304016_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 304016_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:44:26.16 -06:06:22.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 3.333 3100303317781995776 101.10954090124 -06.10697565398 13.0595 11.9466 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.333#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 304836_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 304836_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:42:39.12 -02:16:09.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 304878_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 304878_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 305229_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 305229_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:52:55.07 -02:23:04.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)GAIADR2_OUTPUT=# 3.501 3106018510504636160 103.22925868247 -02.38539636749 13.5296 12.9702 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.501#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 305251_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 305251_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:54:23.38 -01:37:01.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 1.748 3112090426029207936 103.59710334630 -01.61731541411 13.2806 12.4210 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.748#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 305301_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 305301_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 305481_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 305481_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:49:36.00 +01:59:10.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 305574_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 305574_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:41:18.57 -00:51:04.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 2.645 3107333114094700416 100.32703194946 -00.85181643927 13.5990 13.1234 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.645#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 305664_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 305664_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 305682_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 305682_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:45:06.15 -00:02:45.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 2.699 3107483330569016576 101.27521621046 -00.04654528542 13.5111 12.9685 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.699#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 306016_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 306016_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:42:03.39 -06:07:19.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 306701_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 306701_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 307175_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 307175_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:47:10.33 -05:37:13.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 2.585 3100436324330257664 101.79278991116 -05.62100639477 13.7323 13.3078 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.585#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 307217_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 307217_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 307705_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 307705_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 308611_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 308611_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:46:12.55 -05:08:49.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 3.852 3100657291808314112 101.55197132706 -05.14813242199 13.6082 12.7719 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.852#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 308699_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 308699_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:56:43.12 +02:11:50.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 308898_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 308898_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:39:25.05 +00:07:09.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 0.981 3119729764098083584 099.85426175068 +00.11897430785 13.7172 12.9279 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.981#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 309007_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 309007_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 309059_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 309059_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:46:20.37 -05:15:21.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 2.837 3100651210134669056 101.58485367391 -05.25670435408 13.8422 13.2498 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.837#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 309322_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 309322_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 07:01:10.29 -01:01:15.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 3.131 3112567987734134144 105.29366963077 -01.02124268361 13.7541 13.2446 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.131#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 309341_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 309341_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 309397_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 309397_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 309401_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 309401_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 309437_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 309437_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 309706_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 309706_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 309790_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 309790_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 309894_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 309894_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 07:00:53.30 +02:12:19.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 3.743 3115684141125661184 105.22312254508 +02.20541996486 13.5853 12.6957 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.743#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 310028_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 310028_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 310160_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 310160_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
Rejecting candidate due to large distance (8.9") between the two second-epoch detections
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Considering the candidate 310572_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 310572_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 310597_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 310597_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 07:01:26.78 -00:55:29.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 2.245 3112570461635443584 105.36207810215 -00.92448145232 13.7792 12.9935 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.245#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 310716_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 310716_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:43:55.49 -05:04:01.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 2.536 3100716802874635136 100.98061063149 -05.06745965125 14.0739 13.7942 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.536#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 310748_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 310748_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:51:26.31 -02:20:36.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 2.825 3106030429041323008 102.85927994532 -02.34428815611 13.6111 12.7372 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.825#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 311131_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 311131_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:42:46.53 -02:44:16.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 2.400 3106508927049985280 100.69338451398 -02.73839649824 13.7626 13.2404 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.400#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 311265_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 311265_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:55:24.44 -05:54:31.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 311387_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 311387_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 311414_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 311414_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 311502_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 311502_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 311605_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 311605_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 311874_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 311874_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 311903_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 311903_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:48:20.54 -00:31:48.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 311926_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 311926_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 312014_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 312014_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 312179_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 312179_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 312720_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 312720_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:41:21.11 -01:43:20.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 5.187 3106831942950099584 100.33652100745 -01.72233248144 13.6881 12.6456 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.187#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 312966_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 312966_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 312971_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 312971_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 313223_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 313223_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 313310_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 313310_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:41:05.51 -05:41:10.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 3.582 3100575683127182848 100.27197276181 -05.68650192790 13.9287 13.3780 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.582#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 313344_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 313344_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 07:06:54.06 +02:10:47.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 313631_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 313631_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:40:26.02 -01:49:07.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 5.033 3106835447643595264 100.10754055648 -01.81981189803 13.5127 12.5464 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.033#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 313936_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 313936_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:48:43.99 -05:54:27.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 2.202 3100366264824580480 102.18279250022 -05.90788495291 13.4790 12.3244 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.202#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 313956_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 313956_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 07:03:06.93 +01:49:29.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 314014_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 314014_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:54:23.00 -02:46:57.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 3.398 3105945010722645376 103.59538251039 -02.78344079194 13.4180 12.3250 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.398#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 314159_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 314159_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 314201_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 314201_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 314327_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 314327_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:55:58.77 -01:36:01.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 1.882 3112099187762874112 103.99454201873 -01.60068098726 13.8572 13.1918 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.882#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 314345_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 314345_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 314417_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 314417_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 314535_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 314535_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:48:21.03 -03:11:22.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.00, MAG_FAINT_SEARCH_LIMIT=13.98)GAIADR2_OUTPUT=# 1.817 3105495173029126528 102.08747105884 -03.18998084017 13.8439 13.1397 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.817#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 315008_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 315008_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 315100_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 315100_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 07:08:04.44 -01:43:43.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 1.100 3109233104548149120 107.01874958326 -01.72878742697 13.9560 13.4650 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.100#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 315121_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 315121_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 315169_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 315169_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 315280_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 315280_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 315298_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 315298_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:53:45.43 +01:25:43.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 3.268 3114076418906304512 103.43838803221 +01.42863147043 14.0414 13.1455 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.268#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 315502_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 315502_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:36:32.44 -03:35:55.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 4.790 3104844850559457792 099.13443358317 -03.59975014338 14.0155 13.4377 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.790#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 315632_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 315632_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:53:13.89 -04:35:50.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 2.582 3102106757370145024 103.30765488832 -04.59815503995 14.0964 13.6831 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.582#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 315752_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 315752_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 315870_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 315870_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:37:09.70 -01:09:03.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 3.523 3118943231029708032 099.29057638008 -01.15179883888 14.0683 13.4931 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.523#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 316008_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 316008_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 316071_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 316071_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:47:09.59 -05:17:19.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 4.055 3100639871420927872 101.78975441255 -05.28971896782 13.7735 12.8711 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.055#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 316396_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 316396_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:53:56.47 -04:43:54.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 2.411 3102055458280756864 103.48505444976 -04.73232095785 14.0018 13.4206 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.411#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 316578_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 316578_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:42:30.92 -06:04:22.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 1.420 3100477590376003456 100.62876710199 -06.07316657315 14.0485 13.2618 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.420#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 316632_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 316632_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:49:38.86 +00:36:41.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 4.786 3113619949783427072 102.41144535065 +00.61020120759 13.8962 12.9867 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.786#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 316684_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 316684_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 316927_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 316927_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:45:33.86 -00:26:18.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 4.434 3107451723910491520 101.39020146722 -00.43924863840 14.0394 13.6227 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.434#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 317042_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 317042_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 317251_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 317251_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 317324_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 317324_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 317818_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 317818_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:44:19.70 +01:40:46.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 0.918 3125999729156583424 101.08214986352 +01.67994066543 13.9960 13.1111 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.918#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 318087_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 318087_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:50:36.99 -01:46:53.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 3.387 3106322662908980736 102.65406281871 -01.78241089868 14.1429 13.7557 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.387#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 318266_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 318266_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 318300_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 318300_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 07:06:14.81 -04:55:28.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 3.125 3101470827337246464 106.56132619080 -04.92539118273 13.9219 13.2405 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.125#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 318322_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 318322_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 07:03:39.40 -00:16:04.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 4.010 3112714776834452352 105.91520285602 -00.26824174127 13.2419 11.2621 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.010#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 318323_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 318323_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:52:34.69 +00:32:32.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.25, MAG_FAINT_SEARCH_LIMIT=14.23)GAIADR2_OUTPUT=# 4.874 3113580985840503296 103.14371971951 +00.54139619495 14.0748 13.2086 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.874#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 318411_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 318411_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:39:08.72 -03:48:10.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 3.373 3104098655825331328 099.78608026695 -03.80376338268 13.9078 13.3117 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.373#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 318439_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 318439_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 318472_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 318472_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:51:34.20 -02:33:16.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 2.689 3106011535478207360 102.89197053929 -02.55502747934 14.0434 13.2003 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.689#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 318481_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 318481_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 318512_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 318512_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 318696_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 318696_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:37:19.19 +00:16:57.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 2.378 3119703612040020480 099.32944778134 +00.28213637175 12.2889 10.7282 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.378#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 318708_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 318708_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 318756_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 318756_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 319013_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 319013_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 319015_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 319015_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 319089_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 319089_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:46:13.93 -05:27:30.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 0.622 3100630594291784192 101.55802271223 -05.45858847386 14.0725 13.1686 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.622#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 319114_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 319114_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 319341_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 319341_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:54:17.81 -04:54:48.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 2.941 3102036148108303488 103.57398469743 -04.91417479959 14.1319 13.6028 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.941#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 319409_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 319409_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 319428_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 319428_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:40:22.41 +01:18:20.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 2.943 3125881084978463744 100.09324944831 +01.30494231969 14.2492 13.7501 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.943#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 319472_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 319472_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:47:14.66 -03:39:05.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 0.767 3105452708691209216 101.81087051013 -03.65148798860 13.4646 12.2211 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.767#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 319603_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 319603_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 319606_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 319606_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 319740_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 319740_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 319744_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 319744_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:46:57.55 -02:12:27.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 3.091 3106176389201065728 101.73968461197 -02.20840746904 13.9082 12.8701 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.091#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 319799_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 319799_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:51:51.95 -04:03:47.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)GAIADR2_OUTPUT=# 2.703 3102342980571017472 102.96630269222 -04.06398447247 14.2492 13.7474 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.703#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 319893_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 319893_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 320037_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 320037_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 320135_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 320135_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:52:27.32 -05:52:44.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 3.244 3101108916207784960 103.11340523708 -05.87976646569 14.0840 13.5136 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.244#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 320833_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 320833_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 321580_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 321580_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:47:28.96 -01:01:26.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 5.619 3107173165213600896 101.86916799478 -01.02454829849 12.9061 10.7625 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.619#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 321994_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 321994_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 322331_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 322331_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 322528_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 322528_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:52:49.19 -00:35:16.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 3.680 3113160903679411200 103.20592279624 -00.58825520483 14.3206 13.2574 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.680#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 322642_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 322642_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:33:29.09 +01:58:41.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 4.752 3120965610869943424 098.36990336847 +01.97793607089 13.8185 12.3775 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.752#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 322812_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 322812_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:38:53.39 -00:49:17.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 1.810 3119330641377186688 099.72224575617 -00.82187219144 14.2480 13.7440 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.810#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 322813_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 322813_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 07:07:12.09 -06:01:38.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 322896_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 322896_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 322917_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 322917_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 322997_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 322997_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:44:43.22 -02:06:01.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 3.301 3106941413077711360 101.17994342396 -02.10121165387 14.0609 13.1706 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.301#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 323103_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 323103_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:46:39.60 -05:23:53.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 3.056 3100637122641982848 101.66459513421 -05.39894167980 13.9070 13.0179 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.056#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 323104_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 323104_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 323318_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 323318_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 323362_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 323362_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:53:27.11 -00:36:03.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 3.382 3112409524919590528 103.36248731965 -00.60181293285 14.0759 13.0152 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.382#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 323576_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 323576_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 323611_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 323611_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:53:28.75 -01:29:00.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 3.116 3112283459041486208 103.36949685641 -01.48428601164 14.4878 13.6125 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.116#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 323612_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 323612_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 323802_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 323802_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:55:10.95 -02:44:23.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 2.778 3102967022139607040 103.79503428501 -02.74027510327 14.4639 13.4643 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.778#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 323844_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 323844_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 323982_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 323982_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 324068_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 324068_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 324122_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 324122_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:40:26.54 +00:57:19.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 3.407 3119846621567805824 100.11047117625 +00.95442139653 14.6530 14.0850 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.407#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 324149_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 324149_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 324180_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 324180_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:54:03.53 +00:49:28.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 2.262 3113967807774483072 103.51442571846 +00.82388324853 14.4966 13.9552 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.262#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 324236_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 324236_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:59:10.21 +00:11:47.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 2.936 3112944162448397312 104.79212639846 +00.19585363024 14.5982 13.9301 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.936#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 324255_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 324255_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 07:05:05.46 +00:40:06.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 2.177 3114335147735937408 106.27237447948 +00.66805364881 14.6115 14.2516 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.177#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 324319_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 324319_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 324376_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 324376_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:43:53.62 +01:01:51.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 4.483 3125817485103519104 100.97233472643 +01.03021641492 14.4856 13.9817 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.483#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 324402_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 324402_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 324588_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 324588_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 324635_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 324635_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:34:54.36 +01:23:53.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 2.668 3120676855925773696 098.72578573357 +01.39802428046 13.2177 11.7991 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.668#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 324726_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 324726_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 324837_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 324837_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:39:18.11 -00:00:48.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 2.201 3119634037865932160 099.82526587339 -00.01402463254 14.4432 13.6701 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.201#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 324851_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 324851_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 324867_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 324867_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:52:02.28 -02:18:02.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 2.054 3106034041105617152 103.00903540639 -02.30088714513 14.6243 14.1363 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.054#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 324889_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 324889_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:45:47.55 -05:31:37.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 3.329 3100628670147004928 101.44764529420 -05.52773644973 14.3075 13.4068 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.329#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 324924_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 324924_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:54:34.39 -01:09:19.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 3.465 3112325648499548032 103.64279549227 -01.15626921023 14.5400 13.9947 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.465#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 324937_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 324937_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 07:07:17.60 -05:11:21.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 2.200 3053411586406203264 106.82354465304 -05.18990697635 14.6259 14.0440 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.200#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 324955_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 324955_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 324975_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 324975_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 325080_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 325080_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 325086_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 325086_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:52:03.98 -01:15:27.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 3.508 3112347436873213568 103.01632428710 -01.25860600229 14.6296 14.1000 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.508#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 325103_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 325103_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:53:42.71 -03:34:09.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 2.255 3102757187218414848 103.42776419882 -03.56981790922 14.6457 14.1472 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.255#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 325119_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 325119_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 325177_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 325177_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:59:35.47 -02:41:59.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 3.451 3108904969046047360 104.89739831317 -02.70062439642 14.7562 14.0932 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.451#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 325242_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 325242_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:42:14.27 +00:33:25.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 2.435 3119586827586571520 100.55985850799 +00.55662135578 14.6759 13.7369 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.435#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 325303_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 325303_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 07:00:01.78 -04:09:59.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)GAIADR2_OUTPUT=# 1.068 3101805010147493760 105.00723389503 -04.16662310365 14.5636 14.0323 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.068#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 325319_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 325319_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:57:45.99 -05:16:43.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 2.512 3101213919567915136 104.44138425122 -05.27926642880 14.5939 14.0088 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.512#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 325346_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 325346_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:54:21.94 -05:47:10.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 2.167 3101077786285387392 103.59129929362 -05.78678487524 14.7841 14.2050 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.167#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 325369_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 325369_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 325388_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 325388_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 325395_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 325395_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 07:05:26.02 -02:19:26.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.75, MAG_FAINT_SEARCH_LIMIT=14.73)GAIADR2_OUTPUT=# 2.356 3108810204889213440 106.35814706162 -02.32470763478 14.4457 13.9271 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.356#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 325420_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 325420_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:55:03.39 -01:05:17.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.83, MAG_FAINT_SEARCH_LIMIT=14.81)GAIADR2_OUTPUT=# 2.787 3112332937064073984 103.76372557634 -01.08894097571 14.7477 14.3918 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.787#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 325463_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 325463_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:53:53.75 +00:13:41.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 1.283 3113369810888452480 103.47377810593 +00.22785911128 14.7770 14.1477 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.283#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 325476_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
Preparing report for the candidate 325476_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
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Considering the candidate 325536_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 325536_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:56:56.91 +00:03:11.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 2.541 3112926742060801536 104.23687588539 +00.05258959081 14.3367 13.3942 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.541#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 325541_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 325541_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 07:06:37.49 -03:34:46.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 3.750 3107814562749495552 106.65548848873 -03.58044852747 14.6207 13.9759 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.750#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 325567_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 325567_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 07:06:57.96 -05:35:57.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.83, MAG_FAINT_SEARCH_LIMIT=14.81)GAIADR2_OUTPUT=# 2.890 3053324965503140096 106.74095525306 -05.59989769107 14.5506 13.9903 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.890#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 47889_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 47889_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:44:47.60 -05:17:44.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 121122_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 121122_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 07:09:13.64 -02:21:30.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31804_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 31804_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:37:53.20 -05:55:15.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 228912_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033
The candidate 228912_fd_Mon-02-Q2b1x1_2026-04-17_21-40-32_20.00sec_-4.90C_LIGHT_0033 did not pass the final checks
**** FOUND 06:50:00.78 +01:46:33.6 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 8s
make_report_in_HTML.sh TOTAL: 261s
Prepared the HTML report for the field Mon-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
06:58:00.73 -02:49:00.6
06:51:06.77 +00:00:46.3
06:48:41.98 +01:13:23.8
06:57:19.93 -01:46:09.5
06:56:43.20 -02:17:38.1
06:57:06.93 -02:14:44.4
06:51:04.90 -05:28:54.9
06:44:19.61 -00:03:11.9
07:02:46.35 -02:13:12.5
07:03:28.05 -02:23:32.4
06:51:11.53 -02:22:11.3
07:05:45.68 -02:32:45.0
07:04:23.82 -02:15:18.7
07:09:30.12 -03:52:34.9
06:45:11.86 +00:14:16.3
06:55:13.28 -00:26:47.2
06:58:39.30 -01:55:27.6
06:46:31.19 +01:08:35.5
07:05:42.85 -01:37:23.4
06:53:43.53 -01:58:43.1
06:46:42.28 -05:47:35.0
06:56:27.52 -01:27:43.7
07:03:37.09 -00:12:39.0
06:53:04.50 -05:33:24.2
06:54:05.54 -01:51:48.0
06:41:52.88 -05:13:08.1
06:50:49.29 -01:23:56.0
06:57:48.57 -05:46:55.0
06:57:06.75 -00:31:47.2
07:04:35.41 -03:16:30.8
07:02:23.60 -01:34:43.1
07:03:24.29 -03:02:35.8
06:50:23.98 -01:20:43.3
07:05:05.73 -03:34:36.8
07:06:31.63 +01:08:37.9
06:45:27.12 -05:18:37.3
07:03:39.79 -04:38:24.3
06:54:41.06 -02:07:02.4
07:09:26.68 -02:33:07.1
07:09:10.35 -05:50:46.0
06:51:10.52 +01:05:58.6
07:07:06.92 +01:40:00.1
06:53:36.80 -02:31:47.8
06:44:18.20 -05:27:36.0
07:09:10.47 -01:30:23.4
06:48:31.65 -04:05:33.1
06:35:07.44 -03:03:04.1
07:07:51.45 -05:47:00.4
06:58:59.39 -04:37:56.6
07:07:47.32 -05:40:39.7
06:59:00.62 -01:40:01.8
06:54:34.45 -00:35:22.8
06:55:06.32 -06:05:45.5
06:44:39.67 +00:10:06.1
06:55:27.13 -01:16:22.7
07:08:43.26 -05:05:30.1
06:54:48.44 +00:23:17.3
06:56:22.04 -00:53:12.1
06:58:35.49 -04:20:27.6
06:49:56.20 -02:40:54.5
06:42:33.28 -03:28:06.5
06:58:50.15 -04:41:11.4
07:09:39.49 -01:21:49.7
07:04:04.99 -02:22:45.1
07:04:24.69 -04:44:39.0
06:48:53.16 +01:49:30.3
07:04:16.79 -03:01:37.7
07:08:37.34 +00:17:24.8
06:49:07.18 -01:40:18.1
06:59:43.80 +00:17:10.6
07:01:28.22 -05:15:06.9
06:41:27.10 -01:19:02.6
06:51:48.75 -04:02:32.8
06:45:17.56 +00:43:40.0
06:43:36.85 -04:25:03.7
06:53:41.41 -00:33:48.8
06:51:18.24 -01:23:07.4
06:51:34.28 -01:39:23.7
06:44:50.59 +01:05:43.0
06:57:35.69 +01:13:52.7
06:49:55.98 -02:17:03.3
06:57:27.81 -05:05:45.2
06:47:41.07 +00:31:31.3
06:57:52.60 -02:41:33.6
06:44:57.64 -02:51:42.3
06:50:41.54 -00:31:46.7
06:48:56.99 -03:30:58.6
06:35:21.96 -05:17:36.8
06:50:59.50 +00:13:39.3
06:38:52.49 +01:12:23.7
06:49:24.59 -00:56:18.3
07:04:51.60 -02:12:05.3
06:55:15.95 +00:20:57.6
06:53:08.15 -00:50:30.9
06:48:12.12 -00:19:01.3
06:55:11.33 -05:51:22.4
06:41:40.26 -00:36:38.5
06:41:56.37 +00:16:57.0
06:55:14.14 -00:30:56.5
06:50:53.22 -04:59:03.0
06:52:52.51 -00:06:53.4
06:57:11.70 -01:07:45.3
06:52:51.01 -02:20:52.3
06:59:33.93 -00:46:32.6
06:55:00.91 -01:15:41.1
06:53:47.34 -02:38:45.0
06:47:46.48 -02:22:19.8
06:55:50.71 -02:12:29.2
06:59:10.80 -01:18:51.9
06:52:28.67 -04:22:30.7
06:48:04.32 -01:54:53.6
06:59:46.67 -02:22:13.3
06:58:42.23 -04:00:11.4
07:07:15.25 -02:45:46.0
06:45:56.03 -00:30:36.6
06:52:02.69 +01:24:01.6
06:48:22.55 +01:01:07.8
06:59:59.05 -04:07:58.7
07:00:01.70 +00:36:59.4
06:54:25.12 -00:23:50.9
07:09:25.72 -02:13:08.8
06:57:56.62 -02:44:56.8
06:58:34.71 -01:38:24.5
06:54:05.57 -02:52:11.0
07:00:33.29 -04:38:08.3
06:44:09.11 -03:39:06.0
07:04:31.75 +01:55:09.0
06:42:37.18 +00:32:21.4
06:55:25.32 +00:38:47.4
07:04:58.84 -05:16:05.6
06:52:33.58 -03:04:56.0
06:57:19.42 -02:37:59.7
06:55:39.19 -01:03:40.6
06:49:52.39 +01:17:47.6
06:51:19.61 -01:48:30.6
06:50:02.97 -01:11:02.9
########### Completed Mon-02-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
06:58:00.73 -02:49:00.6
06:51:06.77 +00:00:46.3
06:48:41.98 +01:13:23.8
06:57:19.93 -01:46:09.5
06:56:43.20 -02:17:38.1
06:57:06.93 -02:14:44.4
06:51:04.90 -05:28:54.9
06:44:19.61 -00:03:11.9
07:02:46.35 -02:13:12.5
07:03:28.05 -02:23:32.4
06:51:11.53 -02:22:11.3
07:05:45.68 -02:32:45.0
07:04:23.82 -02:15:18.7
07:09:30.12 -03:52:34.9
06:45:11.86 +00:14:16.3
06:55:13.28 -00:26:47.2
06:58:39.30 -01:55:27.6
06:46:31.19 +01:08:35.5
07:05:42.85 -01:37:23.4
06:53:43.53 -01:58:43.1
06:46:42.28 -05:47:35.0
06:56:27.52 -01:27:43.7
07:03:37.09 -00:12:39.0
06:53:04.50 -05:33:24.2
06:54:05.54 -01:51:48.0
06:41:52.88 -05:13:08.1
06:50:49.29 -01:23:56.0
06:57:48.57 -05:46:55.0
06:57:06.75 -00:31:47.2
07:04:35.41 -03:16:30.8
07:02:23.60 -01:34:43.1
07:03:24.29 -03:02:35.8
06:50:23.98 -01:20:43.3
07:05:05.73 -03:34:36.8
07:06:31.63 +01:08:37.9
06:45:27.12 -05:18:37.3
07:03:39.79 -04:38:24.3
06:54:41.06 -02:07:02.4
07:09:26.68 -02:33:07.1
07:09:10.35 -05:50:46.0
06:51:10.52 +01:05:58.6
07:07:06.92 +01:40:00.1
06:53:36.80 -02:31:47.8
06:44:18.20 -05:27:36.0
07:09:10.47 -01:30:23.4
06:48:31.65 -04:05:33.1
06:35:07.44 -03:03:04.1
07:07:51.45 -05:47:00.4
06:58:59.39 -04:37:56.6
07:07:47.32 -05:40:39.7
06:59:00.62 -01:40:01.8
06:54:34.45 -00:35:22.8
06:55:06.32 -06:05:45.5
06:44:39.67 +00:10:06.1
06:55:27.13 -01:16:22.7
07:08:43.26 -05:05:30.1
06:54:48.44 +00:23:17.3
06:56:22.04 -00:53:12.1
06:58:35.49 -04:20:27.6
06:49:56.20 -02:40:54.5
06:42:33.28 -03:28:06.5
06:58:50.15 -04:41:11.4
07:09:39.49 -01:21:49.7
07:04:04.99 -02:22:45.1
07:04:24.69 -04:44:39.0
06:48:53.16 +01:49:30.3
07:04:16.79 -03:01:37.7
07:08:37.34 +00:17:24.8
06:49:07.18 -01:40:18.1
06:59:43.80 +00:17:10.6
07:01:28.22 -05:15:06.9
06:41:27.10 -01:19:02.6
06:51:48.75 -04:02:32.8
06:45:17.56 +00:43:40.0
06:43:36.85 -04:25:03.7
06:53:41.41 -00:33:48.8
06:51:18.24 -01:23:07.4
06:51:34.28 -01:39:23.7
06:44:50.59 +01:05:43.0
06:57:35.69 +01:13:52.7
06:49:55.98 -02:17:03.3
06:57:27.81 -05:05:45.2
06:47:41.07 +00:31:31.3
06:57:52.60 -02:41:33.6
06:44:57.64 -02:51:42.3
06:50:41.54 -00:31:46.7
06:48:56.99 -03:30:58.6
06:35:21.96 -05:17:36.8
06:50:59.50 +00:13:39.3
06:38:52.49 +01:12:23.7
06:49:24.59 -00:56:18.3
07:04:51.60 -02:12:05.3
06:55:15.95 +00:20:57.6
06:53:08.15 -00:50:30.9
06:48:12.12 -00:19:01.3
06:55:11.33 -05:51:22.4
06:41:40.26 -00:36:38.5
06:41:56.37 +00:16:57.0
06:55:14.14 -00:30:56.5
06:50:53.22 -04:59:03.0
06:52:52.51 -00:06:53.4
06:57:11.70 -01:07:45.3
06:52:51.01 -02:20:52.3
06:59:33.93 -00:46:32.6
06:55:00.91 -01:15:41.1
06:53:47.34 -02:38:45.0
06:47:46.48 -02:22:19.8
06:55:50.71 -02:12:29.2
06:59:10.80 -01:18:51.9
06:52:28.67 -04:22:30.7
06:48:04.32 -01:54:53.6
06:59:46.67 -02:22:13.3
06:58:42.23 -04:00:11.4
07:07:15.25 -02:45:46.0
06:45:56.03 -00:30:36.6
06:52:02.69 +01:24:01.6
06:48:22.55 +01:01:07.8
06:59:59.05 -04:07:58.7
07:00:01.70 +00:36:59.4
06:54:25.12 -00:23:50.9
07:09:25.72 -02:13:08.8
06:57:56.62 -02:44:56.8
06:58:34.71 -01:38:24.5
06:54:05.57 -02:52:11.0
07:00:33.29 -04:38:08.3
06:44:09.11 -03:39:06.0
07:04:31.75 +01:55:09.0
06:42:37.18 +00:32:21.4
06:55:25.32 +00:38:47.4
07:04:58.84 -05:16:05.6
06:52:33.58 -03:04:56.0
06:57:19.42 -02:37:59.7
06:55:39.19 -01:03:40.6
06:49:52.39 +01:17:47.6
06:51:19.61 -01:48:30.6
06:50:02.97 -01:11:02.9
###################################################################################
06:58:00.73 -02:49:00.6 -- not an asteroid (will add it to exclusion list)
06:51:06.77 +00:00:46.3 -- not an asteroid (will add it to exclusion list)
06:48:41.98 +01:13:23.8 -- not an asteroid (will add it to exclusion list)
06:57:19.93 -01:46:09.5 -- not an asteroid (will add it to exclusion list)
06:56:43.20 -02:17:38.1 -- not an asteroid (will add it to exclusion list)
06:57:06.93 -02:14:44.4 -- not an asteroid (will add it to exclusion list)
06:51:04.90 -05:28:54.9 -- not an asteroid (will add it to exclusion list)
06:44:19.61 -00:03:11.9 -- not an asteroid (will add it to exclusion list)
07:02:46.35 -02:13:12.5 -- not an asteroid (will add it to exclusion list)
07:03:28.05 -02:23:32.4 -- not an asteroid (will add it to exclusion list)
06:51:11.53 -02:22:11.3 -- not an asteroid (will add it to exclusion list)
07:05:45.68 -02:32:45.0 -- not an asteroid (will add it to exclusion list)
07:04:23.82 -02:15:18.7 -- not an asteroid (will add it to exclusion list)
07:09:30.12 -03:52:34.9 -- not an asteroid (will add it to exclusion list)
06:45:11.86 +00:14:16.3 -- not an asteroid (will add it to exclusion list)
06:55:13.28 -00:26:47.2 -- not an asteroid (will add it to exclusion list)
06:58:39.30 -01:55:27.6 -- not an asteroid (will add it to exclusion list)
06:46:31.19 +01:08:35.5 -- not an asteroid (will add it to exclusion list)
07:05:42.85 -01:37:23.4 -- not an asteroid (will add it to exclusion list)
06:53:43.53 -01:58:43.1 -- not an asteroid (will add it to exclusion list)
06:46:42.28 -05:47:35.0 -- not an asteroid (will add it to exclusion list)
06:56:27.52 -01:27:43.7 -- not an asteroid (will add it to exclusion list)
07:03:37.09 -00:12:39.0 -- not an asteroid (will add it to exclusion list)
06:53:04.50 -05:33:24.2 -- not an asteroid (will add it to exclusion list)
06:54:05.54 -01:51:48.0 -- not an asteroid (will add it to exclusion list)
06:41:52.88 -05:13:08.1 -- not an asteroid (will add it to exclusion list)
06:50:49.29 -01:23:56.0 -- not an asteroid (will add it to exclusion list)
06:57:48.57 -05:46:55.0 -- not an asteroid (will add it to exclusion list)
06:57:06.75 -00:31:47.2 -- not an asteroid (will add it to exclusion list)
07:04:35.41 -03:16:30.8 -- not an asteroid (will add it to exclusion list)
07:02:23.60 -01:34:43.1 -- not an asteroid (will add it to exclusion list)
07:03:24.29 -03:02:35.8 -- not an asteroid (will add it to exclusion list)
06:50:23.98 -01:20:43.3 -- not an asteroid (will add it to exclusion list)
07:05:05.73 -03:34:36.8 -- not an asteroid (will add it to exclusion list)
07:06:31.63 +01:08:37.9 -- not an asteroid (will add it to exclusion list)
06:45:27.12 -05:18:37.3 -- not an asteroid (will add it to exclusion list)
07:03:39.79 -04:38:24.3 -- not an asteroid (will add it to exclusion list)
06:54:41.06 -02:07:02.4 -- not an asteroid (will add it to exclusion list)
07:09:26.68 -02:33:07.1 -- not an asteroid (will add it to exclusion list)
07:09:10.35 -05:50:46.0 -- not an asteroid (will add it to exclusion list)
06:51:10.52 +01:05:58.6 -- not an asteroid (will add it to exclusion list)
07:07:06.92 +01:40:00.1 -- not an asteroid (will add it to exclusion list)
06:53:36.80 -02:31:47.8 -- not an asteroid (will add it to exclusion list)
06:44:18.20 -05:27:36.0 -- not an asteroid (will add it to exclusion list)
07:09:10.47 -01:30:23.4 -- not an asteroid (will add it to exclusion list)
06:48:31.65 -04:05:33.1 -- not an asteroid (will add it to exclusion list)
06:35:07.44 -03:03:04.1 -- not an asteroid (will add it to exclusion list)
07:07:51.45 -05:47:00.4 -- not an asteroid (will add it to exclusion list)
06:58:59.39 -04:37:56.6 -- not an asteroid (will add it to exclusion list)
07:07:47.32 -05:40:39.7 -- not an asteroid (will add it to exclusion list)
06:59:00.62 -01:40:01.8 -- not an asteroid (will add it to exclusion list)
06:54:34.45 -00:35:22.8 -- not an asteroid (will add it to exclusion list)
06:55:06.32 -06:05:45.5 -- not an asteroid (will add it to exclusion list)
06:44:39.67 +00:10:06.1 -- not an asteroid (will add it to exclusion list)
06:55:27.13 -01:16:22.7 -- not an asteroid (will add it to exclusion list)
07:08:43.26 -05:05:30.1 -- not an asteroid (will add it to exclusion list)
06:54:48.44 +00:23:17.3 -- not an asteroid (will add it to exclusion list)
06:56:22.04 -00:53:12.1 -- not an asteroid (will add it to exclusion list)
06:58:35.49 -04:20:27.6 -- not an asteroid (will add it to exclusion list)
06:49:56.20 -02:40:54.5 -- not an asteroid (will add it to exclusion list)
06:42:33.28 -03:28:06.5 -- not an asteroid (will add it to exclusion list)
06:58:50.15 -04:41:11.4 -- not an asteroid (will add it to exclusion list)
07:09:39.49 -01:21:49.7 -- not an asteroid (will add it to exclusion list)
07:04:04.99 -02:22:45.1 -- not an asteroid (will add it to exclusion list)
07:04:24.69 -04:44:39.0 -- not an asteroid (will add it to exclusion list)
06:48:53.16 +01:49:30.3 -- not an asteroid (will add it to exclusion list)
07:04:16.79 -03:01:37.7 -- not an asteroid (will add it to exclusion list)
07:08:37.34 +00:17:24.8 -- not an asteroid (will add it to exclusion list)
06:49:07.18 -01:40:18.1 -- not an asteroid (will add it to exclusion list)
06:59:43.80 +00:17:10.6 -- not an asteroid (will add it to exclusion list)
07:01:28.22 -05:15:06.9 -- not an asteroid (will add it to exclusion list)
06:41:27.10 -01:19:02.6 -- not an asteroid (will add it to exclusion list)
06:51:48.75 -04:02:32.8 -- not an asteroid (will add it to exclusion list)
06:45:17.56 +00:43:40.0 -- not an asteroid (will add it to exclusion list)
06:43:36.85 -04:25:03.7 -- not an asteroid (will add it to exclusion list)
06:53:41.41 -00:33:48.8 -- not an asteroid (will add it to exclusion list)
06:51:18.24 -01:23:07.4 -- not an asteroid (will add it to exclusion list)
06:51:34.28 -01:39:23.7 -- not an asteroid (will add it to exclusion list)
06:44:50.59 +01:05:43.0 -- not an asteroid (will add it to exclusion list)
06:57:35.69 +01:13:52.7 -- not an asteroid (will add it to exclusion list)
06:49:55.98 -02:17:03.3 -- not an asteroid (will add it to exclusion list)
06:57:27.81 -05:05:45.2 -- not an asteroid (will add it to exclusion list)
06:47:41.07 +00:31:31.3 -- not an asteroid (will add it to exclusion list)
06:57:52.60 -02:41:33.6 -- not an asteroid (will add it to exclusion list)
06:44:57.64 -02:51:42.3 -- not an asteroid (will add it to exclusion list)
06:50:41.54 -00:31:46.7 -- not an asteroid (will add it to exclusion list)
06:48:56.99 -03:30:58.6 -- not an asteroid (will add it to exclusion list)
06:35:21.96 -05:17:36.8 -- not an asteroid (will add it to exclusion list)
06:50:59.50 +00:13:39.3 -- not an asteroid (will add it to exclusion list)
06:38:52.49 +01:12:23.7 -- not an asteroid (will add it to exclusion list)
06:49:24.59 -00:56:18.3 -- not an asteroid (will add it to exclusion list)
07:04:51.60 -02:12:05.3 -- not an asteroid (will add it to exclusion list)
06:55:15.95 +00:20:57.6 -- not an asteroid (will add it to exclusion list)
06:53:08.15 -00:50:30.9 -- not an asteroid (will add it to exclusion list)
06:48:12.12 -00:19:01.3 -- not an asteroid (will add it to exclusion list)
06:55:11.33 -05:51:22.4 -- not an asteroid (will add it to exclusion list)
06:41:40.26 -00:36:38.5 -- not an asteroid (will add it to exclusion list)
06:41:56.37 +00:16:57.0 -- not an asteroid (will add it to exclusion list)
06:55:14.14 -00:30:56.5 -- not an asteroid (will add it to exclusion list)
06:50:53.22 -04:59:03.0 -- not an asteroid (will add it to exclusion list)
06:52:52.51 -00:06:53.4 -- not an asteroid (will add it to exclusion list)
06:57:11.70 -01:07:45.3 -- not an asteroid (will add it to exclusion list)
06:52:51.01 -02:20:52.3 -- not an asteroid (will add it to exclusion list)
06:59:33.93 -00:46:32.6 -- not an asteroid (will add it to exclusion list)
06:55:00.91 -01:15:41.1 -- not an asteroid (will add it to exclusion list)
06:53:47.34 -02:38:45.0 -- not an asteroid (will add it to exclusion list)
06:47:46.48 -02:22:19.8 -- not an asteroid (will add it to exclusion list)
06:55:50.71 -02:12:29.2 -- not an asteroid (will add it to exclusion list)
06:59:10.80 -01:18:51.9 -- not an asteroid (will add it to exclusion list)
06:52:28.67 -04:22:30.7 -- not an asteroid (will add it to exclusion list)
06:48:04.32 -01:54:53.6 -- not an asteroid (will add it to exclusion list)
06:59:46.67 -02:22:13.3 -- not an asteroid (will add it to exclusion list)
06:58:42.23 -04:00:11.4 -- not an asteroid (will add it to exclusion list)
07:07:15.25 -02:45:46.0 -- not an asteroid (will add it to exclusion list)
06:45:56.03 -00:30:36.6 -- not an asteroid (will add it to exclusion list)
06:52:02.69 +01:24:01.6 -- not an asteroid (will add it to exclusion list)
06:48:22.55 +01:01:07.8 -- not an asteroid (will add it to exclusion list)
06:59:59.05 -04:07:58.7 -- not an asteroid (will add it to exclusion list)
07:00:01.70 +00:36:59.4 -- not an asteroid (will add it to exclusion list)
06:54:25.12 -00:23:50.9 -- not an asteroid (will add it to exclusion list)
07:09:25.72 -02:13:08.8 -- not an asteroid (will add it to exclusion list)
06:57:56.62 -02:44:56.8 -- not an asteroid (will add it to exclusion list)
06:58:34.71 -01:38:24.5 -- not an asteroid (will add it to exclusion list)
06:54:05.57 -02:52:11.0 -- not an asteroid (will add it to exclusion list)
07:00:33.29 -04:38:08.3 -- not an asteroid (will add it to exclusion list)
06:44:09.11 -03:39:06.0 -- not an asteroid (will add it to exclusion list)
07:04:31.75 +01:55:09.0 -- not an asteroid (will add it to exclusion list)
06:42:37.18 +00:32:21.4 -- not an asteroid (will add it to exclusion list)
06:55:25.32 +00:38:47.4 -- not an asteroid (will add it to exclusion list)
07:04:58.84 -05:16:05.6 -- not an asteroid (will add it to exclusion list)
06:52:33.58 -03:04:56.0 -- not an asteroid (will add it to exclusion list)
06:57:19.42 -02:37:59.7 -- not an asteroid (will add it to exclusion list)
06:55:39.19 -01:03:40.6 -- not an asteroid (will add it to exclusion list)
06:49:52.39 +01:17:47.6 -- not an asteroid (will add it to exclusion list)
06:51:19.61 -01:48:30.6 -- not an asteroid (will add it to exclusion list)
06:50:02.97 -01:11:02.9 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
06:35:07.44 -03:03:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:35:21.96 -05:17:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:38:52.49 +01:12:23.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:27.10 -01:19:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:40.26 -00:36:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:52.88 -05:13:08.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:56.37 +00:16:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:33.28 -03:28:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:37.18 +00:32:21.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:36.85 -04:25:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:09.11 -03:39:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:18.20 -05:27:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:19.61 -00:03:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:39.67 +00:10:06.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:50.59 +01:05:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:57.64 -02:51:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:11.86 +00:14:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:17.56 +00:43:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:27.12 -05:18:37.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:56.03 -00:30:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:31.19 +01:08:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:42.28 -05:47:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:41.07 +00:31:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:46.48 -02:22:19.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:04.32 -01:54:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:12.12 -00:19:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:22.55 +01:01:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:31.65 -04:05:33.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:41.98 +01:13:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:53.16 +01:49:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:56.99 -03:30:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:07.18 -01:40:18.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:24.59 -00:56:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:52.39 +01:17:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:55.98 -02:17:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:56.20 -02:40:54.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:02.97 -01:11:02.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:23.98 -01:20:43.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:41.54 -00:31:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:49.29 -01:23:56.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:53.22 -04:59:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:59.50 +00:13:39.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:04.90 -05:28:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:06.77 +00:00:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:10.52 +01:05:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:11.53 -02:22:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:18.24 -01:23:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:19.61 -01:48:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:34.28 -01:39:23.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:48.75 -04:02:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:02.69 +01:24:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:28.67 -04:22:30.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:33.58 -03:04:56.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:51.01 -02:20:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:52.51 -00:06:53.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:04.50 -05:33:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:08.15 -00:50:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:36.80 -02:31:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:41.41 -00:33:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:43.53 -01:58:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:47.34 -02:38:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:05.54 -01:51:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:05.57 -02:52:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:25.12 -00:23:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:34.45 -00:35:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:41.06 -02:07:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:48.44 +00:23:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:00.91 -01:15:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:06.32 -06:05:45.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:11.33 -05:51:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:13.28 -00:26:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:14.14 -00:30:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:15.95 +00:20:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:25.32 +00:38:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:27.13 -01:16:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:39.19 -01:03:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:50.71 -02:12:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:22.04 -00:53:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:27.52 -01:27:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:43.20 -02:17:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:06.75 -00:31:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:06.93 -02:14:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:11.70 -01:07:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:19.42 -02:37:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:19.93 -01:46:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:27.81 -05:05:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:35.69 +01:13:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:48.57 -05:46:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:52.60 -02:41:33.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:56.62 -02:44:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:00.73 -02:49:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:34.71 -01:38:24.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:35.49 -04:20:27.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:39.30 -01:55:27.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:42.23 -04:00:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:50.15 -04:41:11.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:59.39 -04:37:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:00.62 -01:40:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:10.80 -01:18:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:33.93 -00:46:32.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:43.80 +00:17:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:46.67 -02:22:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:59.05 -04:07:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:01.70 +00:36:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:33.29 -04:38:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:28.22 -05:15:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:23.60 -01:34:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:46.35 -02:13:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:24.29 -03:02:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:28.05 -02:23:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:37.09 -00:12:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:39.79 -04:38:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:04.99 -02:22:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:16.79 -03:01:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:23.82 -02:15:18.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:24.69 -04:44:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:31.75 +01:55:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:35.41 -03:16:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:51.60 -02:12:05.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:58.84 -05:16:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:05.73 -03:34:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:42.85 -01:37:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:45.68 -02:32:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:31.63 +01:08:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:06.92 +01:40:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:15.25 -02:45:46.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:47.32 -05:40:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:51.45 -05:47:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:37.34 +00:17:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:43.26 -05:05:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:10.35 -05:50:46.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:10.47 -01:30:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:25.72 -02:13:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:26.68 -02:33:07.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:30.12 -03:52:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:39.49 -01:21:49.7 -- 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)
06:35:07.44 -03:03:04.1 -- not a known variable star
06:35:21.96 -05:17:36.8 -- not a known variable star
06:38:52.49 +01:12:23.7 -- not a known variable star
06:41:27.10 -01:19:02.6 -- a known variable star
06:41:40.26 -00:36:38.5 -- not a known variable star
06:41:52.88 -05:13:08.1 -- not a known variable star
06:41:56.37 +00:16:57.0 -- not a known variable star
06:42:33.28 -03:28:06.5 -- not a known variable star
06:42:37.18 +00:32:21.4 -- not a known variable star
06:43:36.85 -04:25:03.7 -- a known variable star
06:44:09.11 -03:39:06.0 -- not a known variable star
06:44:18.20 -05:27:36.0 -- not a known variable star
06:44:19.61 -00:03:11.9 -- not a known variable star
06:44:39.67 +00:10:06.1 -- a known variable star
06:44:50.59 +01:05:43.0 -- not a known variable star
06:44:57.64 -02:51:42.3 -- not a known variable star
06:45:11.86 +00:14:16.3 -- not a known variable star
06:45:17.56 +00:43:40.0 -- not a known variable star
06:45:27.12 -05:18:37.3 -- not a known variable star
06:45:56.03 -00:30:36.6 -- not a known variable star
06:46:31.19 +01:08:35.5 -- not a known variable star
06:46:42.28 -05:47:35.0 -- not a known variable star
06:47:41.07 +00:31:31.3 -- not a known variable star
06:47:46.48 -02:22:19.8 -- not a known variable star
06:48:04.32 -01:54:53.6 -- not a known variable star
06:48:12.12 -00:19:01.3 -- a known variable star
06:48:22.55 +01:01:07.8 -- not a known variable star
06:48:31.65 -04:05:33.1 -- a known variable star
06:48:41.98 +01:13:23.8 -- not a known variable star
06:48:53.16 +01:49:30.3 -- a known variable star
06:48:56.99 -03:30:58.6 -- not a known variable star
06:49:07.18 -01:40:18.1 -- not a known variable star
06:49:24.59 -00:56:18.3 -- not a known variable star
06:49:52.39 +01:17:47.6 -- not a known variable star
06:49:55.98 -02:17:03.3 -- not a known variable star
06:49:56.20 -02:40:54.5 -- not a known variable star
06:50:02.97 -01:11:02.9 -- not a known variable star
06:50:23.98 -01:20:43.3 -- not a known variable star
06:50:41.54 -00:31:46.7 -- not a known variable star
06:50:49.29 -01:23:56.0 -- not a known variable star
06:50:53.22 -04:59:03.0 -- not a known variable star
06:50:59.50 +00:13:39.3 -- not a known variable star
06:51:04.90 -05:28:54.9 -- a known variable star
06:51:06.77 +00:00:46.3 -- not a known variable star
06:51:10.52 +01:05:58.6 -- not a known variable star
06:51:11.53 -02:22:11.3 -- not a known variable star
06:51:18.24 -01:23:07.4 -- a known variable star
06:51:19.61 -01:48:30.6 -- not a known variable star
06:51:34.28 -01:39:23.7 -- not a known variable star
06:51:48.75 -04:02:32.8 -- a known variable star
06:52:02.69 +01:24:01.6 -- not a known variable star
06:52:28.67 -04:22:30.7 -- not a known variable star
06:52:33.58 -03:04:56.0 -- a known variable star
06:52:51.01 -02:20:52.3 -- not a known variable star
06:52:52.51 -00:06:53.4 -- not a known variable star
06:53:04.50 -05:33:24.2 -- not a known variable star
06:53:08.15 -00:50:30.9 -- a known variable star
06:53:36.80 -02:31:47.8 -- a known variable star
06:53:41.41 -00:33:48.8 -- a known variable star
06:53:43.53 -01:58:43.1 -- not a known variable star
06:53:47.34 -02:38:45.0 -- not a known variable star
06:54:05.54 -01:51:48.0 -- not a known variable star
06:54:05.57 -02:52:11.0 -- not a known variable star
06:54:25.12 -00:23:50.9 -- not a known variable star
06:54:34.45 -00:35:22.8 -- not a known variable star
06:54:41.06 -02:07:02.4 -- a known variable star
06:54:48.44 +00:23:17.3 -- a known variable star
06:55:00.91 -01:15:41.1 -- a known variable star
06:55:06.32 -06:05:45.5 -- not a known variable star
06:55:11.33 -05:51:22.4 -- not a known variable star
06:55:13.28 -00:26:47.2 -- not a known variable star
06:55:14.14 -00:30:56.5 -- not a known variable star
06:55:15.95 +00:20:57.6 -- not a known variable star
06:55:25.32 +00:38:47.4 -- not a known variable star
06:55:27.13 -01:16:22.7 -- a known variable star
06:55:39.19 -01:03:40.6 -- not a known variable star
06:55:50.71 -02:12:29.2 -- not a known variable star
06:56:22.04 -00:53:12.1 -- a known variable star
06:56:27.52 -01:27:43.7 -- not a known variable star
06:56:43.20 -02:17:38.1 -- a known variable star
06:57:06.75 -00:31:47.2 -- a known variable star
06:57:06.93 -02:14:44.4 -- not a known variable star
06:57:11.70 -01:07:45.3 -- a known variable star
06:57:19.42 -02:37:59.7 -- not a known variable star
06:57:19.93 -01:46:09.5 -- a known variable star
06:57:27.81 -05:05:45.2 -- not a known variable star
06:57:35.69 +01:13:52.7 -- a known variable star
06:57:48.57 -05:46:55.0 -- not a known variable star
06:57:52.60 -02:41:33.6 -- not a known variable star
06:57:56.62 -02:44:56.8 -- not a known variable star
06:58:00.73 -02:49:00.6 -- not a known variable star
06:58:34.71 -01:38:24.5 -- not a known variable star
06:58:35.49 -04:20:27.6 -- not a known variable star
06:58:39.30 -01:55:27.6 -- not a known variable star
06:58:42.23 -04:00:11.4 -- not a known variable star
06:58:50.15 -04:41:11.4 -- not a known variable star
06:58:59.39 -04:37:56.6 -- not a known variable star
06:59:00.62 -01:40:01.8 -- not a known variable star
06:59:10.80 -01:18:51.9 -- not a known variable star
06:59:33.93 -00:46:32.6 -- not a known variable star
06:59:43.80 +00:17:10.6 -- a known variable star
06:59:46.67 -02:22:13.3 -- not a known variable star
06:59:59.05 -04:07:58.7 -- not a known variable star
07:00:01.70 +00:36:59.4 -- not a known variable star
07:00:33.29 -04:38:08.3 -- not a known variable star
07:01:28.22 -05:15:06.9 -- a known variable star
07:02:23.60 -01:34:43.1 -- not a known variable star
07:02:46.35 -02:13:12.5 -- not a known variable star
07:03:24.29 -03:02:35.8 -- not a known variable star
07:03:28.05 -02:23:32.4 -- not a known variable star
07:03:37.09 -00:12:39.0 -- not a known variable star
07:03:39.79 -04:38:24.3 -- not a known variable star
07:04:04.99 -02:22:45.1 -- a known variable star
07:04:16.79 -03:01:37.7 -- not a known variable star
07:04:23.82 -02:15:18.7 -- a known variable star
07:04:24.69 -04:44:39.0 -- not a known variable star
07:04:31.75 +01:55:09.0 -- not a known variable star
07:04:35.41 -03:16:30.8 -- a known variable star
07:04:51.60 -02:12:05.3 -- not a known variable star
07:04:58.84 -05:16:05.6 -- not a known variable star
07:05:05.73 -03:34:36.8 -- not a known variable star
07:05:42.85 -01:37:23.4 -- not a known variable star
07:05:45.68 -02:32:45.0 -- a known variable star
07:06:31.63 +01:08:37.9 -- a known variable star
07:07:06.92 +01:40:00.1 -- not a known variable star
07:07:15.25 -02:45:46.0 -- not a known variable star
07:07:47.32 -05:40:39.7 -- not a known variable star
07:07:51.45 -05:47:00.4 -- a known variable star
07:08:37.34 +00:17:24.8 -- not a known variable star
07:08:43.26 -05:05:30.1 -- a known variable star
07:09:10.35 -05:50:46.0 -- a known variable star
07:09:10.47 -01:30:23.4 -- a known variable star
07:09:25.72 -02:13:08.8 -- not a known variable star
07:09:26.68 -02:33:07.1 -- not a known variable star
07:09:30.12 -03:52:34.9 -- a known variable star
07:09:39.49 -01:21:49.7 -- not a known variable star
Found 101 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
136 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 136 (excluding asteroids and hot pixels, 101 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)2461148.61096332 -observatory V36
00:18:39.10 -00:51:07.7 Mercury (-0.0mag)
03:19:00.54 +18:37:53.5 Venus (-3.9mag)
00:23:49.95 +01:31:24.2 Mars (1.2mag)
07:13:36.83 +22:44:36.4 Jupiter (-2.1mag)
00:30:07.09 +00:54:48.7 Saturn (0.9mag)
03:48:08.72 +19:48:54.6 Uranus (5.8mag)
00:11:06.86 -00:13:38.8 Neptune (7.8mag)
20:33:50.53 -22:52:42.7 Pluto (14.5mag)
02:06:15.16 +17:06:49.6 Moon (-8.3mag)
-rw-r--r-- 1 apache apache 362 Apr 17 22:09 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461148.61096332:
07:13:43.35 +22:44:24.1 Io (5.8mag)
07:13:28.19 +22:44:52.9 Europa (5.9mag)
07:13:23.74 +22:44:58.4 Ganymede (5.4mag)
07:14:03.30 +22:43:35.2 Callisto (6.6mag)
07:16:51.35 +22:31:16.2 Himalia (15.3mag)
07:13:36.18 +22:44:35.5 Thebe (16.2mag)
07:17:05.37 +23:01:34.3 Elara (17.3mag)
07:12:38.33 +23:23:30.5 Pasiphae (17.4mag)
07:21:53.66 +22:42:49.7 Carme (18.5mag)
00:30:00.38 +00:55:15.2 Titan (8.8mag)
00:30:12.20 +00:54:56.3 Rhea (10.1mag)
00:29:43.78 +00:54:37.8 Iapetus (11.5mag)
00:30:07.25 +00:55:16.1 Hyperion (14.8mag)
00:31:42.28 +01:03:23.1 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 17 22:09 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461148.61096332:
15:47:28.54 -17:40:23.5 JWST
19:13:21.67 +13:40:27.8 Chandra
07:51:33.34 -34:02:00.5 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 17 22:09 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461148.61096332 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:52:48.72 -28:54:16.7 13.9mag P/2010 H2 (Vales)
05:08:16.31 -69:33:48.4 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:32:54.95 +31:27:07.7 17.2mag C/2017 K2 (PANSTARRS)
17:30:12.14 +10:47:46.1 17.6mag C/2021 G2 (ATLAS)
23:10:46.00 +29:18:50.5 17.1mag C/2022 E2 (ATLAS)
04:31:42.38 +26:05:42.3 16.0mag C/2022 N2 (PANSTARRS)
09:03:54.44 +32:01:37.4 16.2mag C/2022 QE78 (ATLAS)
08:31:25.43 +00:04:02.8 17.3mag C/2022 R6 (PANSTARRS)
18:53:12.10 +18:42:29.4 17.6mag C/2023 A3 (Tsuchinshan-ATLAS)
15:39:58.31 -11:29:25.9 17.5mag P/2023 B1 (PANSTARRS)
09:06:41.99 -11:32:55.8 17.7mag C/2023 F3 (ATLAS)
21:56:16.53 +63:01:56.0 17.5mag C/2023 H5 (Lemmon)
19:17:17.45 -03:46:12.2 14.1mag C/2023 R1 (PANSTARRS)
21:27:28.50 +86:12:22.8 17.8mag C/2023 X2 (Lemmon)
06:18:57.04 +63:30:20.4 17.2mag C/2024 A1 (ATLAS)
05:17:44.66 +18:59:08.5 11.2mag C/2024 E1 (Wierzchos)
16:17:53.46 +06:44:07.4 17.4mag C/2024 G6 (ATLAS)
20:21:22.04 +15:51:07.7 14.6mag C/2024 J3 (ATLAS)
03:28:16.55 -22:04:02.4 16.3mag C/2024 T5 (ATLAS)
05:18:31.20 +44:46:25.6 17.7mag C/2025 J1 (Borisov)
13:30:07.22 +46:46:22.8 15.3mag C/2025 L1 (ATLAS)
03:28:39.00 -26:32:46.6 17.8mag C/2025 Q3 (ATLAS)
00:05:05.18 +17:40:05.6 8.2mag C/2025 R3 (PANSTARRS)
12:53:12.62 +03:08:20.0 17.4mag C/2025 Y1 (ATLAS)
03:44:04.78 +02:25:06.4 13.9mag C/2026 A1 (MAPS)
00:05:30.25 +37:35:53.2 14.6mag C/2026 B2 (Sun-Gao)
18:47:02.36 -09:36:17.4 11.7mag 10P/Tempel
14:57:26.00 +02:58:54.2 14.2mag 24P/Schaumasse
11:02:15.77 -01:27:35.2 15.7mag 29P/Schwassmann-Wachmann
18:01:29.03 -09:32:04.5 18.0mag 40P/Vaisala
10:37:32.35 -03:56:11.6 16.9mag 43P/Wolf-Harrington
01:51:56.67 +17:50:45.0 17.2mag 47P/Ashbrook-Jackson
07:14:42.06 +36:33:23.1 17.0mag 63P/Wild
23:31:43.87 -11:11:57.7 15.7mag 65P/Gunn
04:08:55.97 +21:58:12.4 15.9mag 76P/West-Kohoutek-Ikemura
01:10:15.29 +08:38:31.0 14.3mag 78P/Gehrels
23:09:20.62 -08:45:59.2 14.6mag 88P/Howell
02:16:24.62 +21:11:55.6 15.1mag 93P/Lovas
04:58:49.38 +32:23:51.2 16.2mag 123P/West-Hartley
08:30:54.87 +37:23:17.9 16.2mag 124P/Mrkos
02:36:29.32 +14:36:14.1 16.4mag 128P/Shoemaker-Holt
02:51:41.14 +14:44:50.9 17.5mag 131P/Mueller
01:37:19.61 +13:56:52.1 10.6mag 141P/Machholz
01:45:56.41 +05:39:46.2 10.6mag 141P-A/Machholz
00:30:16.17 +01:30:16.4 12.6mag 141P-D/Machholz
02:16:24.85 +07:25:17.5 17.8mag 141P-I/Machholz
01:08:16.64 -00:27:41.9 15.0mag 162P/SidingSpring
14:47:41.73 +00:08:25.4 17.7mag 210P/Christensen
21:44:51.05 -10:56:30.1 17.7mag 218P/LINEAR
17:16:59.92 -13:40:38.6 16.1mag 235P/LINEAR
05:39:03.88 +34:51:07.8 16.8mag 240P/NEAT
07:39:33.97 -04:56:34.3 17.7mag 242P/Spahr
22:22:11.20 -20:24:34.7 17.8mag 260P/McNaught
02:02:31.26 +20:59:22.1 18.0mag 295P/LINEAR
15:41:47.57 +07:07:35.7 17.5mag 391P/Kowalski
07:35:02.32 +21:22:15.5 17.7mag 450P/LONEOS
05:38:58.38 +44:54:33.9 17.5mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 17 22:09 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
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
17:21:59.44 -38:54:04.60 2026-04-14.4 15.15
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
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
-rw-r--r-- 1 apache apache 5.8K Apr 17 22:09 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
00:43:38.36 +41:15:32.4 PNV J00433836+4115324 2026-04-08.079 17.2mag
15:41:11.68 +59:18:26.8 TCP J15411168+5918268 2026-04-12.9625 19.2mag
-rw-r--r-- 1 apache apache 188K Apr 17 22:09 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
17:52:44.230 +56:55:19.06 AT 2026jfc 2026-03-27.87 20.98
14:01:07.200 +03:10:48.03 AT 2026jfb 2026-04-05.73 21.73
13:47:01.080 +02:47:45.39 AT 2026jfa 2026-03-24.91 20.68
17:11:20.724 -17:18:29.68 AT 2026jez 2026-04-04.38 17.507
03:59:36.404 -57:03:28.57 AT 2026jey 2026-04-05.01 18.79
03:57:56.301 -54:05:57.45 AT 2026jex 2026-04-08.01 19.148
10:30:49.649 -08:04:36.38 AT 2026jew 2026-04-07.87 19.144
12:27:21.393 -28:22:09.12 AT 2026jev 2026-04-10.19 18.809
17:40:25.287 +05:08:20.96 AT 2026jeu 2026-04-05.42 17.65
08:35:16.434 -77:00:48.01 AT 2026jet 2026-04-09.11 19.072
21:53:03.051 -16:55:33.84 AT 2026jes 2026-04-10.38 17.345
00:36:19.401 -83:06:05.82 AT 2026jer 2026-04-08.40 18.473
22:08:10.236 -21:46:23.75 AT 2026jeq 2026-04-10.39 18.259
21:34:17.331 -33:37:48.49 AT 2026jep 2026-04-10.39 18.372
16:56:26.248 +04:54:42.94 AT 2026jeo 2026-04-10.42 18.3645
08:10:18.680 +34:40:45.43 AT 2026jen 2026-04-05.17 20.6002
10:14:46.220 +16:03:20.00 AT 2026jem 2026-04-07.20 20.5179
09:08:33.148 +56:28:29.17 AT 2026jel 2026-04-09.15 19.5877
08:06:59.814 +72:49:07.23 AT 2026jek 2026-04-05.15 20.127
10:17:15.279 +45:17:14.78 AT 2026jej 2026-04-08.19 20.2002
-rw-r--r-- 1 apache apache 30K Apr 17 22:09 tns_transients_list.txt
