This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud
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
ATO J100.4676-05.5163,2461149.6131,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J100.4676-05.5163 20260419.1131 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3101436192711109632,2461149.6131,10.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3101436192711109632 20260419.1131 10.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3125630499409158144,2461149.6131,11.69,0.05,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
Gaia DR3 3125630499409158144 20260419.1131 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108734574801210240,2461149.6131,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108734574801210240 20260419.1131 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6131,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1131 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J102.5098+01.1390,2461149.6131,13.72,0.05,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
ATO J102.5098+01.1390 20260419.1131 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 3109096833825051904,2461149.6131,13.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109096833825051904 20260419.1131 13.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.7800-02.7699,2461149.6131,13.71,0.05,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
ATO J106.7800-02.7699 20260419.1131 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,2461149.6131,13.70,0.05,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 20260419.1131 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 J103.5364-01.5315,2461149.6131,13.66,0.05,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 J103.5364-01.5315 20260419.1131 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 3053231708868263296,2461149.6131,13.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3053231708868263296 20260419.1131 13.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.1616-02.2261,2461149.6131,13.88,0.05,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
ATO J104.1616-02.2261 20260419.1131 13.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6131,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1131 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J0654398-015601,2461149.6131,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J0654398-015601 20260419.1131 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112299500737047808,2461149.6131,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112299500737047808 20260419.1131 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3105971506383189504,2461149.6131,13.55,0.05,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
Gaia DR3 3105971506383189504 20260419.1131 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
Gaia DR3 3102757389074908544,2461149.6131,13.60,0.05,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
Gaia DR3 3102757389074908544 20260419.1131 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
ATO J102.7395-02.0003,2461149.6131,13.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J102.7395-02.0003 20260419.1131 13.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6131,13.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1131 13.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108851436574453504,2461149.6131,13.45,0.05,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 3108851436574453504 20260419.1131 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 3106566475310188032,2461149.6131,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3106566475310188032 20260419.1131 13.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.2984-01.3857,2461149.6131,13.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J105.2984-01.3857 20260419.1131 13.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.8851+00.9980,2461149.6131,13.59,0.05,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
ATO J101.8851+00.9980 20260419.1131 13.59CV 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
ATO J104.1174-02.9061,2461149.6131,13.39,0.05,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
ATO J104.1174-02.9061 20260419.1131 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 J105.9023-03.3839,2461149.6131,13.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.9023-03.3839 20260419.1131 13.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107171584665401984,2461149.6131,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107171584665401984 20260419.1131 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J065202+0026.7,2461149.6131,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J065202+0026.7 20260419.1131 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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,2461149.6131,13.32,0.05,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 20260419.1131 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
ATO J105.7017-05.4676,2461149.6131,13.43,0.05,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 J105.7017-05.4676 20260419.1131 13.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6131,13.43,0.05,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
target 20260419.1131 13.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3053347333693607040,2461149.6131,13.31,0.05,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
Gaia DR3 3053347333693607040 20260419.1131 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
Gaia DR3 3109186920759226752,2461149.6131,13.35,0.05,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 3109186920759226752 20260419.1131 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
target,2461149.6131,13.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1131 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461149.6131,13.36,0.05,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
VARIABLE_NAME 20260419.1131 13.36CV 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 3100611352837987968,2461149.6131,13.35,0.05,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 3100611352837987968 20260419.1131 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
target,2461149.6131,13.24,0.05,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
target 20260419.1131 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
target,2461149.6131,13.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1131 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.4280-01.9828,2461149.6131,13.30,0.05,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 J103.4280-01.9828 20260419.1131 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 J101.0643-00.0070,2461149.6131,13.29,0.05,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
ATO J101.0643-00.0070 20260419.1131 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 J105.4375-01.1737,2461149.6131,13.09,0.05,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 J105.4375-01.1737 20260419.1131 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
Gaia DR3 3101146368322338688,2461149.6131,13.18,0.05,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 3101146368322338688 20260419.1131 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
Gaia DR3 3112107704678242432,2461149.6131,13.42,0.05,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
Gaia DR3 3112107704678242432 20260419.1131 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 J102.7908-02.3649,2461149.6131,13.39,0.05,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
ATO J102.7908-02.3649 20260419.1131 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
Gaia DR3 3108998839851392768,2461149.6131,13.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108998839851392768 20260419.1131 13.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.3754-00.9507,2461149.6131,13.12,0.05,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 J107.3754-00.9507 20260419.1131 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
ATO J101.6375-01.8671,2461149.6131,13.22,0.05,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
ATO J101.6375-01.8671 20260419.1131 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,2461149.6131,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1131 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 3059427667355169920,2461149.6131,12.99,0.05,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
Gaia DR3 3059427667355169920 20260419.1131 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
ATO J104.6668-01.9250,2461149.6131,13.19,0.05,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
ATO J104.6668-01.9250 20260419.1131 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 3107059954174122624,2461149.6131,13.15,0.05,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
Gaia DR3 3107059954174122624 20260419.1131 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 J104.9950-05.8987,2461149.6131,13.15,0.05,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
ATO J104.9950-05.8987 20260419.1131 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 J104.7533-02.6015,2461149.6131,13.12,0.05,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 J104.7533-02.6015 20260419.1131 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,2461149.6131,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1131 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
ATO J106.9353-03.1808,2461149.6131,12.93,0.05,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
ATO J106.9353-03.1808 20260419.1131 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
target,2461149.6131,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1131 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.3373-03.5634,2461149.6131,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.3373-03.5634 20260419.1131 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3053380868799189632,2461149.6131,12.93,0.05,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 3053380868799189632 20260419.1131 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 3112469585742136064,2461149.6131,13.09,0.05,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
Gaia DR3 3112469585742136064 20260419.1131 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
Gaia DR3 3101335278168470784,2461149.6131,12.98,0.05,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 3101335278168470784 20260419.1131 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 J104.4680-01.7871,2461149.6131,13.18,0.05,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
ATO J104.4680-01.7871 20260419.1131 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
target,2461149.6131,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1131 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6131,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1131 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3101279508008034560,2461149.6131,12.93,0.05,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 3101279508008034560 20260419.1131 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 J106.0207+00.9747,2461149.6131,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.0207+00.9747 20260419.1131 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.9152-04.6412,2461149.6131,12.88,0.05,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
ATO J105.9152-04.6412 20260419.1131 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6131,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1131 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
target,2461149.6131,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1131 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 3114569137555198464,2461149.6131,12.88,0.05,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 3114569137555198464 20260419.1131 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6131,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1131 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 J104.5329-01.2670,2461149.6131,13.04,0.05,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
ATO J104.5329-01.2670 20260419.1131 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
ATO J107.3525-02.5480,2461149.6131,12.86,0.05,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 J107.3525-02.5480 20260419.1131 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,2461149.6131,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1131 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106052732803548160,2461149.6131,12.84,0.05,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 3106052732803548160 20260419.1131 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 J105.5241-02.7611,2461149.6131,12.88,0.05,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
ATO J105.5241-02.7611 20260419.1131 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 J106.6876-01.5149,2461149.6131,12.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.6876-01.5149 20260419.1131 12.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112617946791292672,2461149.6131,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112617946791292672 20260419.1131 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3101503262931004032,2461149.6131,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3101503262931004032 20260419.1131 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107977187391380864,2461149.6131,12.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107977187391380864 20260419.1131 12.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J102.9700-04.4046,2461149.6131,12.69,0.05,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 J102.9700-04.4046 20260419.1131 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
target,2461149.6131,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260419.1131 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107274358943072000,2461149.6131,12.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107274358943072000 20260419.1131 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.3114-06.2236,2461149.6131,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.3114-06.2236 20260419.1131 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J107.1974-03.7119,2461149.6131,12.71,0.05,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
ATO J107.1974-03.7119 20260419.1131 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 3053304074782543488,2461149.6131,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3053304074782543488 20260419.1131 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3105924742777831040,2461149.6131,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3105924742777831040 20260419.1131 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109235166132304128,2461149.6131,12.53,0.05,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 3109235166132304128 20260419.1131 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 3053213021476196992,2461149.6131,12.59,0.05,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 3053213021476196992 20260419.1131 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
target,2461149.6131,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1131 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3109336454339492608,2461149.6131,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109336454339492608 20260419.1131 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6131,12.64,0.05,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
target 20260419.1131 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
Gaia DR3 3101503262931006720,2461149.6131,12.61,0.05,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
Gaia DR3 3101503262931006720 20260419.1131 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 3113171417759759232,2461149.6131,12.63,0.05,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 3113171417759759232 20260419.1131 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.1845-04.1464,2461149.6131,12.38,0.05,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
ATO J106.1845-04.1464 20260419.1131 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3059453162280747520,2461149.6131,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3059453162280747520 20260419.1131 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3105965733946504448,2461149.6131,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3105965733946504448 20260419.1131 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.7071-03.3905,2461149.6131,12.37,0.05,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
ATO J106.7071-03.3905 20260419.1131 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112954191193204096,2461149.6131,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112954191193204096 20260419.1131 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J070702.55-015739.5,2461149.6131,12.16,0.05,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
ASASSN-V J070702.55-015739.5 20260419.1131 12.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J098.7797-03.0546,2461149.6131,12.43,0.05,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 J098.7797-03.0546 20260419.1131 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.9390-02.6747,2461149.6131,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J106.9390-02.6747 20260419.1131 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107032775621691520,2461149.6131,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3107032775621691520 20260419.1131 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107979214615799680,2461149.6131,12.01,0.05,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 3107979214615799680 20260419.1131 12.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.7305-03.0153,2461149.6131,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J104.7305-03.0153 20260419.1131 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3108867959307360128,2461149.6131,11.96,0.05,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 3108867959307360128 20260419.1131 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3101821880779349888,2461149.6131,11.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3101821880779349888 20260419.1131 11.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J101.1090+01.9830,2461149.6131,11.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J101.1090+01.9830 20260419.1131 11.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113487424272581760,2461149.6131,10.52,0.05,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 3113487424272581760 20260419.1131 10.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113144097467624576,2461149.6131,10.97,0.05,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 3113144097467624576 20260419.1131 10.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3101857958506347264,2461149.6131,11.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3101857958506347264 20260419.1131 11.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3114765366021631360,2461149.6131,11.69,0.05,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
Gaia DR3 3114765366021631360 20260419.1131 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx695048,2461149.6131,11.85,0.05,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
DocumentRef: VOTx695048 20260419.1131 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx691655,2461149.6131,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx691655 20260419.1131 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106324999372001664,2461149.6131,12.12,0.05,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 3106324999372001664 20260419.1131 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.9752-06.0043,2461149.6131,12.38,0.05,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
ATO J105.9752-06.0043 20260419.1131 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3053416980884797824,2461149.6131,12.48,0.05,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 3053416980884797824 20260419.1131 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 J103.2327-02.3822,2461149.6131,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.2327-02.3822 20260419.1131 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J0654238-013737,2461149.6131,12.62,0.05,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
GDS_J0654238-013737 20260419.1131 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 3112424230887731712,2461149.6131,12.57,0.05,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 20260419.1131 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 J100.9536+01.2405,2461149.6131,12.62,0.05,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
ATO J100.9536+01.2405 20260419.1131 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
ZTF J065448.56+002321.1,2461149.6131,12.55,0.05,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
ZTF J065448.56+002321.1 20260419.1131 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 3109532137349277568,2461149.6131,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109532137349277568 20260419.1131 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3105921684761121152,2461149.6131,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3105921684761121152 20260419.1131 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6131,12.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260419.1131 12.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6131,12.70,0.05,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 20260419.1131 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
Gaia DR3 3126153111029053568,2461149.6131,12.86,0.05,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 3126153111029053568 20260419.1131 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
ATO J104.3550-02.9498,2461149.6131,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.3550-02.9498 20260419.1131 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
TZ Mon,2461149.6131,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
TZ Mon 20260419.1131 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.6490-04.3421,2461149.6131,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.6490-04.3421 20260419.1131 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.2998-03.9607,2461149.6131,12.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J104.2998-03.9607 20260419.1131 12.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.0676-03.0161,2461149.6131,12.78,0.05,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 J106.0676-03.0161 20260419.1131 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3105621277567743360,2461149.6131,12.73,0.05,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 3105621277567743360 20260419.1131 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
target,2461149.6131,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1131 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3105302831513609216,2461149.6131,12.90,0.05,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 3105302831513609216 20260419.1131 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 3053393715036723840,2461149.6131,12.78,0.05,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
Gaia DR3 3053393715036723840 20260419.1131 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3107281540128223104,2461149.6131,12.94,0.05,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 3107281540128223104 20260419.1131 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J100.9776-05.0786,2461149.6131,12.97,0.05,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
ATO J100.9776-05.0786 20260419.1131 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
ATO J102.9043-01.6544,2461149.6131,12.98,0.05,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
ATO J102.9043-01.6544 20260419.1131 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
CoRoT 102806577,2461149.6131,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CoRoT 102806577 20260419.1131 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3100477590376004224,2461149.6131,12.94,0.05,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 3100477590376004224 20260419.1131 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 3125637852391270784,2461149.6131,12.96,0.05,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 3125637852391270784 20260419.1131 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 3119745157261836032,2461149.6131,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3119745157261836032 20260419.1131 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106128697885405184,2461149.6131,13.00,0.05,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
Gaia DR3 3106128697885405184 20260419.1131 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,2461149.6131,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260419.1131 13.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106651897920988800,2461149.6131,12.98,0.05,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 3106651897920988800 20260419.1131 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 3100429448080531584,2461149.6131,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3100429448080531584 20260419.1131 13.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3125607134785759744,2461149.6131,13.06,0.05,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 3125607134785759744 20260419.1131 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 3109656416522583808,2461149.6131,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109656416522583808 20260419.1131 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J099.7529-00.5089,2461149.6131,13.16,0.05,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
ATO J099.7529-00.5089 20260419.1131 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
target,2461149.6131,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1131 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112503842401083904,2461149.6131,13.01,0.05,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 3112503842401083904 20260419.1131 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 3113913996125565440,2461149.6131,13.07,0.05,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 3113913996125565440 20260419.1131 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
Gaia DR3 3103464959174981120,2461149.6131,13.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3103464959174981120 20260419.1131 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3113651900038506752,2461149.6131,13.22,0.05,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 3113651900038506752 20260419.1131 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
ATO J099.6630+01.9547,2461149.6131,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J099.6630+01.9547 20260419.1131 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6131,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1131 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 3126750798678879360,2461149.6131,13.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3126750798678879360 20260419.1131 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6131,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260419.1131 13.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106831938650976384,2461149.6131,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3106831938650976384 20260419.1131 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J106.3566-03.3095,2461149.6131,13.07,0.05,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
ATO J106.3566-03.3095 20260419.1131 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,2461149.6131,13.16,0.05,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
target 20260419.1131 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 3105951818253305728,2461149.6131,13.12,0.05,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 3105951818253305728 20260419.1131 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 3118998932463086720,2461149.6131,13.21,0.05,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
Gaia DR3 3118998932463086720 20260419.1131 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 3105494249614626944,2461149.6131,13.12,0.05,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 3105494249614626944 20260419.1131 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
ATO J103.9421-02.1958,2461149.6131,13.24,0.05,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 J103.9421-02.1958 20260419.1131 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
DocumentRef: VOTx907700,2461149.6131,13.09,0.05,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
DocumentRef: VOTx907700 20260419.1131 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
ATO J100.2049+00.9685,2461149.6131,13.21,0.05,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 J100.2049+00.9685 20260419.1131 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
DocumentRef: VOTx926464,2461149.6131,13.44,0.05,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
DocumentRef: VOTx926464 20260419.1131 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 3105909998152601088,2461149.6131,13.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3105909998152601088 20260419.1131 13.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx939089,2461149.6131,13.28,0.05,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
DocumentRef: VOTx939089 20260419.1131 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 J104.6381-01.6369,2461149.6131,13.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.6381-01.6369 20260419.1131 13.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3106945708044956416,2461149.6131,13.34,0.05,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 3106945708044956416 20260419.1131 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,2461149.6131,13.35,0.05,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 20260419.1131 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 3102956027023684096,2461149.6131,13.34,0.05,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 3102956027023684096 20260419.1131 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
DocumentRef: VOTx958415,2461149.6131,13.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx958415 20260419.1131 13.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx961823,2461149.6131,13.48,0.05,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
DocumentRef: VOTx961823 20260419.1131 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
Gaia DR3 3105590967980076416,2461149.6131,13.53,0.05,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
Gaia DR3 3105590967980076416 20260419.1131 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
GDS_J0655376-053532,2461149.6131,13.34,0.05,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
GDS_J0655376-053532 20260419.1131 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,2461149.6131,13.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1131 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
target,2461149.6131,13.38,0.05,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
target 20260419.1131 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
Gaia DR3 3109579137170282880,2461149.6131,13.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3109579137170282880 20260419.1131 13.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.6452-06.1044,2461149.6131,13.15,0.05,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
ATO J105.6452-06.1044 20260419.1131 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
target,2461149.6131,13.48,0.05,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
target 20260419.1131 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 J102.1827-05.9078,2461149.6131,13.29,0.05,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
ATO J102.1827-05.9078 20260419.1131 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
Gaia DR3 3106229822896913792,2461149.6131,13.39,0.05,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
Gaia DR3 3106229822896913792 20260419.1131 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
GDS_J0641451-005653,2461149.6131,13.68,0.05,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
GDS_J0641451-005653 20260419.1131 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
Gaia DR3 3125762543878388096,2461149.6131,13.46,0.05,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 3125762543878388096 20260419.1131 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
ATO J100.8511-00.4371,2461149.6131,13.62,0.05,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
ATO J100.8511-00.4371 20260419.1131 13.62CV 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 3119565215311245568,2461149.6131,13.62,0.05,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 3119565215311245568 20260419.1131 13.62CV 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 3101752748985728512,2461149.6131,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3101752748985728512 20260419.1131 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3112332249869918080,2461149.6131,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3112332249869918080 20260419.1131 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J103.4522-03.2954,2461149.6131,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J103.4522-03.2954 20260419.1131 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 3101520919530256896,2461149.6131,13.62,0.05,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 3101520919530256896 20260419.1131 13.62CV 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 3108996258570070528,2461149.6131,13.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 3108996258570070528 20260419.1131 13.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6131,13.72,0.05,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 20260419.1131 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 3113218284441983360,2461149.6131,13.67,0.05,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
Gaia DR3 3113218284441983360 20260419.1131 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 J103.0157-00.6017,2461149.6131,13.85,0.05,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
ATO J103.0157-00.6017 20260419.1131 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
target,2461149.6131,13.71,0.05,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 20260419.1131 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 J103.2919-01.6972,2461149.6131,13.88,0.05,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
ATO J103.2919-01.6972 20260419.1131 13.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6131,13.68,0.05,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 20260419.1131 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
## 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: 2461149.61341892 19.04.2026 02:43:09.395 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 13
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): 31001
Objects passed selection criteria: 30874
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 24656.2
Average stars matched: 22359.8 (90.6859 %)
Memory usage VmPeak: 131292 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 Sun Apr 19 06:50:42 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: 2461149.61341892 19.04.2026 02:43:09.395 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 478
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: 209 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): 227783
Objects passed selection criteria: 227057
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: 186281
Average stars matched: 169346 (90.9092 %)
Memory usage VmPeak: 1981732 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 Sun Apr 19 06:57:53 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_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.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_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.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: 2461149.61286255
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_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits'
wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.fits exists and is non-empty
Saving wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.fits to local_wcs_cache/
'wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.fits' -> 'local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.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_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits (1st new image)
verification OK: wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits
Image size: 937.4'x624.3' 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: 06:51:26.184 -01:59:58.68 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 06:51:26.184 -01:59:58.68
Angular distance between the image centers 0.0705 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.fits (2nd new image)
verification OK: wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.fits
Image size: 937.4'x624.3' 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: 06:51:27.480 -01:59:40.96 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 06:51:27.480 -01:59:40.96
Angular distance between the image centers 0.0657 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 06:51:26.184 -01:59:58.68
Second-epoch second image center 06:51:27.480 -01:59:40.96
Angular distance between the image centers 0.00730 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.Y4WneFfc6f
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.YWkvOReUa8
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_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits &> /tmp/tmp.eRVMEY4t1Y
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.fits &> /tmp/tmp.KJNBJCmjhS
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.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 13 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
2.6 pix fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits
2.5 pix fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.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_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits
14.7 mag. fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.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.Y4WneFfc6f (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_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/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.YWkvOReUa8 (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_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/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.eRVMEY4t1Y (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_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.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_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.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_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2851, passed=27868
Got 27868 stars (including 24996 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits.cat
util/solve_plate_with_UCAC5 got 27868 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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 -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 914 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 27393 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
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 -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 929 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(), 27391 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 27392 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.74"
Excluding outliers - 927 stars left (next iteration limit 1018)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.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.KJNBJCmjhS (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_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.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_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.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_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2897, passed=27573
Got 27573 stars (including 24653 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.fits.cat
util/solve_plate_with_UCAC5 got 27573 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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 -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 925 matched stars entering correct_measured_positions(), 912 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.74"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 925 matched stars entering correct_measured_positions(), 27267 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
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 -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 27266 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 27267 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.79"
Excluding outliers - 926 stars left (next iteration limit 1017)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.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_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/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_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/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_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits'
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.fits'
Preparing the HTML report for the field Mon-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out57438.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out51885.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out51890.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out51882.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51891.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55869.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57920.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out58110.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 117s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 4s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51882_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 51882_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51885_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 51885_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:02:02.20 -01:58:18.8 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.00, MAG_FAINT_SEARCH_LIMIT=12.98)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51890_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 51890_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:38:07.45 -01:28:04.1 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=11.02, MAG_FAINT_SEARCH_LIMIT=12.00)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51891_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 51891_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54427_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 54427_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:09:13.63 -02:21:30.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54687_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 54687_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:42:37.27 -03:49:19.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55869_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 55869_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56697_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 56697_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:44:47.51 -05:17:45.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57438_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 57438_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:42:36.15 -02:12:24.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.01, MAG_FAINT_SEARCH_LIMIT=12.99)GAIADR2_OUTPUT=# 1.993 3106608119313089792 100.65078624539 -02.20722417901 11.9774 11.6699 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.993#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57439_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 57439_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:08:45.33 +00:41:48.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57857_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 57857_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:37:55.82 -01:31:33.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57920_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 57920_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58110_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 58110_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 121s
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 ####
06:41:52.25 -05:30:57.4
07:04:59.46 -05:12:08.6
06:44:58.53 +00:57:06.9
07:01:14.75 -02:44:16.9
06:56:48.80 +02:10:37.6
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 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_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.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_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.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_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.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_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits exists and is non-empty
wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.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_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits (1st new image)
verification OK: wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits
Image size: 937.4'x624.3' 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: 06:51:26.184 -01:59:58.68 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 06:51:26.184 -01:59:58.68
Angular distance between the image centers 0.0705 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.fits (2nd new image)
verification OK: wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.fits
Image size: 937.4'x624.3' 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: 06:51:27.480 -01:59:40.96 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 06:51:27.480 -01:59:40.96
Angular distance between the image centers 0.0657 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 06:51:26.184 -01:59:58.68
Second-epoch second image center 06:51:27.480 -01:59:40.96
Angular distance between the image centers 0.00730 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.FHTMC8jEiM
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.ZdbKmbMCAE
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_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits &> /tmp/tmp.4Rdg1p1s4n
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.fits &> /tmp/tmp.2znnthnIYe
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.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 396 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_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits
2.2 pix fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.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_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits
14.0 mag. fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 13.4 (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.FHTMC8jEiM (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_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/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.ZdbKmbMCAE (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_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/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.4Rdg1p1s4n (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_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.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_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.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_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=91, blended=29488, passed=194089
Got 194089 stars (including 164389 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits.cat
util/solve_plate_with_UCAC5 got 194089 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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 -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 930 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(), 911 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 190985 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 -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 190986 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 190988 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
Excluding outliers - 928 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_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.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.2znnthnIYe (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_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.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_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.fits
WCS_IMAGE_NAME=wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.fits
WCS-calibrated image found: wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.fits
Checking if the catalog wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.fits.cat corresponding to the image wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.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_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.fits
WCS catalog name: wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=64, blended=30442, passed=199205
Got 199205 stars (including 168554 good ones) from the SExtractor catalog wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.fits.cat
util/solve_plate_with_UCAC5 got 199205 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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 -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 910 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 195723 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.4)
Done reading UCAC5 zone files...
Matched 928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 195721 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 195721 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Excluding outliers - 928 stars left (next iteration limit 1019)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.fits -region wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.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_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/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_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/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_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.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_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-42-21_20.00sec_-5.00C_LIGHT_0355.fits
Saving fully-calibrated image wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.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_2026-04-18_CI_Mon-02-Q2b1x1_214350_TTUQ2b1x1_2776363_J6KcN6ud/wcs_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356.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
Adding exclusion_list_gaiadr2.txt__out283566.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283586.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283587.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283627.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283690.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283695.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283699.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283700.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283708.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283715.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283716.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283724.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283733.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283748.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283752.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283756.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283774.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283782.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283784.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283785.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283799.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283803.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283820.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283822.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283824.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283835.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283836.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283842.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283851.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283857.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283859.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283890.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283900.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283915.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283928.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283932.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283939.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283940.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283941.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283955.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283956.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283967.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283970.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283983.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out283987.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out284006.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out284017.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out284023.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out284036.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out284041.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out284043.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out284052.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out284056.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out284062.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out284067.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out284077.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out284079.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out284085.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out284091.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out284092.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out284108.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out284119.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out284124.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out284131.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out284136.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out284149.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out293461.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out299763.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out299983.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out300263.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out301673.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out302618.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out302797.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out306155.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out306205.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out306650.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out307017.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out307401.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out307439.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out307982.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out308422.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out308507.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out308872.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out309704.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out309854.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out310361.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out311057.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out311793.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out311818.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out311821.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out312184.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out312215.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out312537.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out312977.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out313055.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out314821.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315190.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315205.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315209.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315210.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315350.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315599.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315846.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out315933.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316070.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316167.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316511.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316667.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out316810.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out318084.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out318143.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out318191.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out319342.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out319993.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out321713.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out321965.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out322318.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out322327.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out322597.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out322657.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out322923.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out322977.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out323144.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out323397.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out323484.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out323601.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out323771.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out323929.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out324064.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out324080.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out324157.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out324166.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out324224.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out324309.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out324407.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out324516.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out324557.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out324589.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out324596.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out324655.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out324678.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out324807.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out324824.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out324842.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out324871.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out324952.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out325010.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out325031.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out325035.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out325070.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out325086.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out325261.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out325288.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out325327.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out283780.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out303595.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out283597.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283600.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
Adding exclusion_list_local.txt__out283618.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283626.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283628.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283641.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283649.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283652.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283670.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283673.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283679.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283712.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283723.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283737.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283740.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283755.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283762.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283769.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283772.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283781.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283791.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283801.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283804.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283807.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283809.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283811.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283813.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283821.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283828.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283831.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283833.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283839.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283843.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283846.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283848.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283849.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283852.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283865.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283873.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283889.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283891.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283892.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283894.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283895.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283907.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283908.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283918.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283922.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283925.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283927.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283937.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283943.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283946.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283950.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283952.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283958.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283963.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283966.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283968.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283969.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283979.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283982.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283985.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283986.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283990.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283992.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out283996.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284007.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284009.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284012.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284013.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284020.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284021.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284029.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284031.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284038.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284047.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284054.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284057.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284059.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284064.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284065.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284066.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284075.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284084.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284093.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284094.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284102.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284111.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284112.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284113.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284115.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284127.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284130.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284132.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284134.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284141.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284145.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out284147.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out286989.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288742.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293473.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out293663.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out294965.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298176.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out298245.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out301270.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out303343.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out303417.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out304739.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out304975.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out305086.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out305192.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out305197.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out305625.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out306726.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out306811.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out307100.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out307306.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out307434.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out307624.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out307637.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out307966.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out308058.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out308956.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out309147.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out310469.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out310518.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out310897.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out311051.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out311062.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out311287.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out311310.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out311764.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out312674.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out312687.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out313020.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out313179.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out313488.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out313548.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out313618.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out314101.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out314250.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out315110.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out315150.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out315332.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out315458.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out315528.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out315874.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316036.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316149.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316211.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316378.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316470.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316489.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316592.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out316927.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out317261.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out317340.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out317390.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out317716.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out318045.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out318946.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out318972.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out318973.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out319760.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out319825.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out319982.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out319988.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out320203.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out320592.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out320636.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out320659.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out320890.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out321064.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out321186.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out321401.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out321406.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out321723.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out322206.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out323300.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out323566.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out323860.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out323950.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out324383.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out324473.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out324533.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out324800.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out324929.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out325094.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out325153.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out325157.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 430s
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: 124s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283566_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 283566_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:05:19.90 -03:25:09.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 2.914 3107879640093284736 106.33231520732 -03.41995959605 14.3892 14.0163 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.914#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283586_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 283586_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:52:13.35 -00:32:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.00, MAG_FAINT_SEARCH_LIMIT=14.98)GAIADR2_OUTPUT=# 3.625 3113175369129362432 103.05532571605 -00.54993354243 14.8929 14.3311 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.625#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283587_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 283587_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:01:20.03 -03:04:44.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 2.431 3108689430408765440 105.33313041221 -03.07950739032 14.7659 14.1168 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.431#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283597_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283597_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283600_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283600_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283607_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283607_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283609_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283609_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283618_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283618_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283626_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283626_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283627_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 283627_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:08:22.34 -05:32:33.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 4.589 3053340599185309824 107.09300747588 -05.54396697811 14.2908 14.0677 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.589#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283628_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283628_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283641_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283641_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283649_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283649_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283652_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283652_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283670_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283670_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283673_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283673_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283679_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283679_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283687_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 283687_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
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Considering the candidate 283690_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 283690_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:09:30.13 -02:28:42.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 3.562 3108408470826506496 107.37515152719 -02.47940951283 14.1083 13.2369 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.562#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283695_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 283695_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:01:19.93 -00:56:41.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 3.239 3112568954105823744 105.33361949851 -00.94546764897 14.2680 13.7804 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.239#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283699_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 283699_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:05:49.85 -01:38:15.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 4.645 3109274679831101184 106.45821982357 -01.63871250965 14.2250 13.4102 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.645#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283700_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 283700_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:46:11.79 +00:50:14.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 2.860 3125567891665421568 101.54879744084 +00.83672062076 14.3349 13.7505 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.860#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283708_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 283708_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:59:25.35 -02:10:12.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)
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Considering the candidate 283712_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283712_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283715_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 283715_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:42:39.15 -02:47:36.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 2.815 3106502604858174720 100.66277420044 -02.79403243674 14.0226 13.0989 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.815#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283716_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 283716_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:44:27.07 -03:16:41.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 1.589 3105675462875645184 101.11279383084 -03.27866373900 14.3570 13.6693 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.589#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283723_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283723_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283724_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 283724_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:56:21.44 -01:51:07.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 3.605 3112021259876395776 104.08879614522 -01.85284537684 14.5108 14.1077 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.605#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283733_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 283733_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:46:59.91 +02:05:47.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 3.135 3126365351133202432 101.74939775405 +02.09563161190 14.0540 13.2075 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.135#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283736_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 283736_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
Rejecting candidate due to large distance (21.3") between the two second-epoch detections
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Considering the candidate 283737_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283737_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283740_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283740_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283746_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 283746_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 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 283748_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 283748_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:03:45.82 -02:37:46.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)
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Considering the candidate 283752_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 283752_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:00:19.05 -05:42:34.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 2.908 3100986183224870272 105.07902539175 -05.71034010852 14.3175 13.7325 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.908#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283755_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283755_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283756_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 283756_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:34:57.09 -00:43:39.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)
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Considering the candidate 283762_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283762_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283769_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283769_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283772_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283772_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283774_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 283774_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:08:58.11 -02:02:48.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 3.225 3109207987580040832 107.24141515231 -02.04726912096 14.2858 13.5687 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.225#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283780_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 283780_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:01:52.88 -02:51:17.9 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)
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Considering the candidate 283781_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283781_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283782_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 283782_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:02:43.65 -02:26:02.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)
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Considering the candidate 283784_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 283784_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:37:56.00 +00:48:04.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 2.746 3119831739505299200 099.48321128109 +00.80041368826 14.1506 13.5830 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.746#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283785_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 283785_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:52:04.69 -05:47:09.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 4.098 3101113382973759744 103.01906948900 -05.78712030010 14.4191 13.7240 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.098#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283791_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283791_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283799_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 283799_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:47:23.66 +01:30:18.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 2.531 3125765567538996864 101.84829729096 +01.50441327626 14.1440 13.7368 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.531#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283801_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283801_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283803_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 283803_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:57:45.64 -04:35:58.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 1.627 3101676264206730240 104.43986579872 -04.59978271368 14.2028 13.8431 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.627#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283804_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283804_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283807_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283807_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283809_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283809_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283811_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283811_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283813_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283813_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283820_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 283820_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:00:08.23 -03:25:02.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 4.250 3102625589420641920 105.03393293605 -03.41834725416 14.0949 13.3743 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.250#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283821_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283821_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283822_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 283822_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:09:18.98 -01:02:03.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)
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Considering the candidate 283824_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 283824_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:44:45.13 -05:42:12.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)
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Considering the candidate 283828_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283828_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283831_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283831_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283833_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283833_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283835_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 283835_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:39:23.69 -00:23:27.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 3.690 3119418293069471360 099.84830254289 -00.39194123631 13.9457 13.3191 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.690#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283836_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 283836_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:39:49.04 +01:09:07.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 3.421 3125872112787850752 099.95380648619 +01.15118133169 14.1561 13.3983 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.421#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283839_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283839_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283842_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 283842_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:08:32.58 -04:52:13.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 3.279 3059428423269301248 107.13498037393 -04.87093591462 13.8481 13.1876 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.279#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283843_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283843_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283846_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283846_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283848_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283848_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283849_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283849_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283851_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 283851_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:53:46.13 -00:14:31.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 3.057 3113269304351579776 103.44210583164 -00.24287080058 14.0933 13.6557 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.057#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283852_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283852_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283857_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 283857_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:01:15.90 +02:06:06.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 2.182 3115491868329337088 105.31592046554 +02.10121341358 14.0937 13.5772 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.182#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283859_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 283859_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:56:16.04 +00:50:25.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 4.509 3113790030488569344 104.06634330768 +00.83937519847 14.0012 13.4666 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.509#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283865_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283865_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283867_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 283867_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:43:14.29 +01:58:17.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 283873_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283873_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283889_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283889_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283890_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 283890_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:49:53.29 +01:01:24.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 2.889 3113667331861561728 102.47196760975 +01.02256213902 13.9973 13.5646 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.889#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283891_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283891_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283892_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283892_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283894_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283894_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283895_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283895_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283900_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 283900_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:00:25.50 -01:23:49.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 3.444 3112164986662186496 105.10684723657 -01.39783089041 14.0627 13.6227 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.444#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283904_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 283904_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
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Considering the candidate 283907_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283907_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283908_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283908_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283915_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 283915_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:06:13.60 -03:55:51.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 2.014 3107588127772486400 106.55629805906 -03.93142166306 13.9663 13.5456 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.014#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283918_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283918_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283922_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283922_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283925_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283925_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283927_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283927_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283928_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 283928_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:48:51.88 +00:01:27.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 2.822 3113451445327095424 102.21594845509 +00.02355261831 13.8506 13.3312 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.822#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283932_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 283932_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:47:02.74 -03:47:43.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 4.307 3105398214146218752 101.76102461712 -03.79643612422 13.8623 13.1274 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.307#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283937_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283937_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283939_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 283939_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:39:29.25 +01:49:48.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 2.251 3126729770517775488 099.87168789424 +01.82948669425 13.5118 12.5826 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.251#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283940_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 283940_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:43:11.65 -02:02:01.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 2.519 3106617259003491456 100.79850991076 -02.03450460142 13.7064 13.1691 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.519#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283941_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 283941_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:05:27.56 -01:00:09.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 2.083 3109568623093291648 106.36453423089 -01.00305075955 13.7684 12.8340 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.083#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283943_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283943_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283946_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283946_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283950_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283950_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283952_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283952_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283955_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 283955_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:38:27.00 -05:35:50.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)
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Considering the candidate 283956_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 283956_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:03:20.18 +01:33:20.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 0.788 3115401055542013568 105.83420033145 +01.55585162026 13.8464 12.8763 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.788#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283958_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283958_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283963_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283963_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283966_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283966_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283967_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 283967_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:53:46.88 +01:14:29.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 3.411 3114016907839549696 103.44545394980 +01.24053236295 13.8689 13.0160 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.411#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 283968_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283968_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283969_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283969_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283970_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 283970_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:05:19.34 -01:29:12.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 3.940 3109468056438096000 106.33034015352 -01.48790042039 13.5034 12.6642 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.940#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283979_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283979_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 283982_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283982_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283983_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 283983_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:49:49.96 +00:33:03.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 2.556 3113616548169343104 102.45804111476 +00.55027335106 13.6126 12.7223 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.556#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283985_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283985_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283986_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283986_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283987_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 283987_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:07:30.90 +01:02:11.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 3.356 3114373248387789312 106.87812752763 +01.03586142044 13.6793 13.2963 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.356#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283990_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283990_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283992_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283992_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 283996_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 283996_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284006_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 284006_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:05:06.15 -04:00:13.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 2.816 3107769203592227584 106.27515859253 -04.00446217511 13.6174 13.0843 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.816#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284007_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 284007_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284009_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 284009_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284012_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 284012_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284013_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 284013_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284017_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 284017_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:09:03.81 -01:19:31.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)
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Considering the candidate 284020_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 284020_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284021_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 284021_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284023_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 284023_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:06:05.21 -05:15:57.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 1.520 3053398529704718976 106.52144410328 -05.26635805752 13.7535 12.8795 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.520#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284029_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 284029_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284031_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 284031_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284036_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 284036_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:07:25.52 +02:12:22.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 2.374 3114795327712115072 106.85615195023 +02.20564379253 13.4253 12.6756 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.374#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284038_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 284038_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284041_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 284041_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:07:06.98 +01:40:00.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 4.040 3114693863405107840 106.77860669604 +01.66587278863 13.6698 13.1945 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.040#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 284043_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 284043_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:52:04.44 -05:53:12.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 1.930 3101108259073557760 103.01829861414 -05.88727505251 13.5348 13.0509 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.930#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284047_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 284047_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284052_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 284052_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:41:44.26 +00:27:30.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 3.401 3119584108871539072 100.43410634763 +00.45760760434 13.7271 13.1248 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.401#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284054_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 284054_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284056_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 284056_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:08:06.99 -02:10:35.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 3.336 3109182630093180160 107.02872493063 -02.17722501208 13.4626 13.0189 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.336#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284057_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 284057_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284059_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 284059_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284062_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 284062_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:40:52.95 -01:58:39.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 3.484 3106817065184077312 100.22043042317 -01.97855920489 13.6217 13.0149 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.484#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284064_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 284064_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284065_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 284065_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284066_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 284066_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284067_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 284067_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:55:04.99 -01:02:55.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 1.991 3112333899136721408 103.77089108376 -01.04932192669 13.4551 12.7464 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.991#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 284075_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 284075_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 284077_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 284077_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:08:42.78 +01:59:44.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.50, MAG_FAINT_SEARCH_LIMIT=13.48)GAIADR2_OUTPUT=# 1.100 3114730692744947456 107.17833101923 +01.99528879820 13.2190 12.4774 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 284079_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 284079_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:53:42.81 -02:56:56.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 2.800 3102933727553341056 103.42803614841 -02.94975585056 13.3565 12.4843 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.800#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284084_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 284084_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284085_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 284085_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:48:49.70 +00:22:42.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284091_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 284091_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:43:16.54 +00:21:47.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284092_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 284092_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:46:12.61 +00:51:09.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 2.783 3125567930324132096 101.55227975245 +00.85185603769 13.4133 12.9328 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.783#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284093_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 284093_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284094_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 284094_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284102_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 284102_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284108_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 284108_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:40:13.61 +01:34:06.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 1.799 3126640293461251840 100.05661954788 +01.56798053311 12.8907 11.9582 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.799#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284111_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 284111_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284112_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 284112_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284113_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 284113_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284115_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 284115_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284119_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 284119_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:42:09.70 -03:38:08.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 1.950 3105548125684846336 100.54031504037 -03.63619866648 12.9583 12.1518 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.950#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284124_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 284124_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:08:33.14 +00:32:15.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 4.420 3114294122208651008 107.13787303785 +00.53631806316 13.1529 12.4015 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.420#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284127_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 284127_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284130_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 284130_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284131_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 284131_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:05:10.99 -00:29:20.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 1.971 3112693400776779520 106.29629603399 -00.48935224730 12.8501 12.4125 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.971#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284132_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 284132_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284133_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 284133_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:51:02.40 +01:07:16.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284134_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 284134_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284136_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 284136_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:52:09.25 +00:34:44.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 2.280 3113585005929929984 103.03834255055 +00.57848204790 12.7509 11.9519 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.280#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284139_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 284139_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:54:08.26 -05:53:00.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284141_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 284141_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284145_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 284145_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284147_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 284147_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284149_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 284149_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:52:43.53 -01:37:06.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.76, MAG_FAINT_SEARCH_LIMIT=12.74)GAIADR2_OUTPUT=# 1.603 3112286517058110720 103.18126310508 -01.61895875764 12.6308 11.9779 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.603#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284150_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 284150_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:53:50.82 +01:53:34.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284151_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 284151_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:56:14.07 -05:00:24.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284152_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 284152_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:04:15.71 -02:22:58.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284153_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 284153_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:08:35.64 +01:46:45.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284158_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 284158_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:06:44.62 -01:25:53.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284159_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 284159_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:07:26.08 -01:50:45.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284163_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 284163_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:08:38.10 -05:29:37.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 284169_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 284169_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:07:49.56 -05:43:08.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 286978_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 286978_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:50:40.17 -00:32:22.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 286989_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 286989_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288621_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 288621_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:51:37.23 +00:26:59.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 288742_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 288742_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289215_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 289215_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:51:39.72 +00:25:33.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 289791_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 289791_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:40:37.71 +00:43:03.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 290474_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 290474_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:40:30.56 -01:04:42.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291024_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 291024_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:04:10.71 -03:14:38.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 291827_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 291827_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:50:41.62 -00:33:42.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293461_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 293461_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:57:39.92 -05:17:24.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.66, MAG_FAINT_SEARCH_LIMIT=12.64)GAIADR2_OUTPUT=# 1.355 3101213777831416960 104.41613637585 -05.29032131842 12.4704 11.6797 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.355#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293473_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 293473_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 293663_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 293663_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 294965_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 294965_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 296666_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 296666_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:50:44.40 -00:31:37.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298176_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 298176_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298245_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 298245_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 298906_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 298906_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:45:00.21 -00:03:30.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 299763_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 299763_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:45:04.74 -01:02:22.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 2.757 3107346681891637888 101.26967865935 -01.04031808691 13.2059 12.6723 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.757#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 299983_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 299983_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:05:01.43 +01:48:37.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 0.900 3114755436055724928 106.25598204354 +01.81022333530 13.0723 12.2193 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.900#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 300263_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 300263_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:34:15.03 -05:19:04.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)GAIADR2_OUTPUT=# 2.525 3103462897582381312 098.56209663853 -05.31829740534 13.0894 12.5053 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.525#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 301270_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 301270_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 301673_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 301673_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:00:51.58 -03:52:04.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 0.895 3101842737140035328 105.21494516568 -03.86819152005 13.1228 12.5967 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.895#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 301914_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 301914_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:43:50.49 +01:35:51.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 302105_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 302105_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:04:34.92 -05:56:30.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 302618_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 302618_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:45:06.19 -00:02:46.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 2.285 3107483330569016576 101.27521621046 -00.04654528542 13.5111 12.9685 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.285#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 302797_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 302797_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:38:54.23 +00:00:13.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 2.564 3119634652045900032 099.72581188348 +00.00294192467 13.1884 12.6963 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.564#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 303138_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 303138_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:42:03.35 -06:07:17.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 303321_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 303321_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:53:07.34 -01:52:41.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 303343_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 303343_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 303417_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 303417_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 303595_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 303595_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:40:19.84 -03:22:49.6 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 303769_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 303769_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:42:39.13 -02:16:09.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 304260_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 304260_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:44:36.03 +01:45:25.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 304739_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 304739_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 304975_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 304975_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 305086_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 305086_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 305192_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 305192_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 305197_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 305197_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 305625_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 305625_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 306155_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 306155_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:46:14.78 -02:18:25.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 4.335 3106174641154272896 101.56114866774 -02.30809529203 13.4455 12.5508 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.335#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 306205_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 306205_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:41:18.57 -00:51:03.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 3.096 3107333114094700416 100.32703194946 -00.85181643927 13.5990 13.1234 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.096#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 306650_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 306650_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:41:58.11 -00:53:39.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 2.204 3107328475530410368 100.49184650310 -00.89496181731 13.1913 12.1887 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.204#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 306719_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 306719_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:44:26.04 -06:06:23.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 306726_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 306726_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 306811_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 306811_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 307017_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 307017_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:52:14.04 -00:06:01.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 3.575 3113331499779778176 103.05834787681 -00.10148142245 13.5344 12.6718 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.575#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 307100_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 307100_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 307306_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 307306_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 307401_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 307401_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:53:59.69 -02:44:17.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 3.631 3105945972795426816 103.49787131933 -02.73864765651 13.4074 12.4613 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.631#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 307434_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 307434_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 307439_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 307439_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:35:50.38 +00:49:55.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 2.590 3120591570757150976 098.95968284379 +00.83145849529 13.5954 13.0905 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.590#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 307624_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 307624_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 307637_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 307637_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 307966_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 307966_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 307982_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 307982_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:41:47.06 -00:16:14.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 3.222 3119468149051361920 100.44582555146 -00.27157940447 13.7130 13.3699 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.222#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 308058_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 308058_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 308422_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 308422_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:40:25.89 -01:49:08.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 2.886 3106835447643595264 100.10754055648 -01.81981189803 13.5127 12.5464 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.886#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 308507_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 308507_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:00:53.18 +02:12:19.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 5.538 3115684141125661184 105.22312254508 +02.20541996486 13.5853 12.6957 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.538#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 308872_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 308872_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:42:29.69 -04:08:22.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 1.454 3105326264854304256 100.62362023901 -04.13992208149 13.6824 12.7988 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 308956_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 308956_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 309147_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 309147_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 309423_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 309423_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:56:43.13 +02:11:51.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 309704_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 309704_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:06:11.82 +00:18:32.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 0.479 3114262610029958784 106.54920449104 +00.30906939611 13.7638 13.2801 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.479#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 309854_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 309854_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:46:20.34 -05:15:20.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 3.655 3100651210134669056 101.58485367391 -05.25670435408 13.8422 13.2498 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.655#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 310361_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 310361_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:46:12.51 -05:08:49.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 3.916 3100657291808314112 101.55197132706 -05.14813242199 13.6082 12.7719 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.916#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 310469_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 310469_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 310518_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 310518_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 310897_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 310897_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 311051_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 311051_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 311057_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 311057_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:44:56.62 +01:18:42.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 5.462 3125922316666768256 101.23503212452 +01.31062814339 13.8014 12.9660 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.462#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 311062_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 311062_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 311287_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 311287_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 311310_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 311310_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 311429_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 311429_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:55:24.45 -05:54:31.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 311668_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 311668_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:48:33.37 +01:51:09.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 311764_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 311764_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 311793_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 311793_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:37:33.26 +01:24:38.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 3.635 3120687370005889280 099.38804092931 +01.40995382945 13.9336 13.3825 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.635#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 311818_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 311818_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:08:49.45 +00:27:15.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 2.365 3114279519319862400 107.20543385668 +00.45405634620 13.8903 13.4119 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.365#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 311821_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 311821_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:35:10.37 -00:43:20.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 4.903 3119206774519517696 098.79348040669 -00.72377880410 14.0197 13.4537 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.903#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 312184_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 312184_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:46:50.66 +01:18:09.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 5.159 3125737976669232256 101.71061901697 +01.30128313633 13.9023 13.1882 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.159#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 312215_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 312215_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:48:20.98 -03:11:21.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 2.938 3105495173029126528 102.08747105884 -03.18998084017 13.8439 13.1397 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.938#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 312537_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 312537_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:01:10.30 -01:01:15.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 2.819 3112567987734134144 105.29366963077 -01.02124268361 13.7541 13.2446 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.819#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 312674_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 312674_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 312687_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 312687_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 312977_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 312977_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:40:05.30 -04:41:38.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 2.546 3103780042268573568 100.02241043894 -04.69454432899 13.8502 13.0386 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.546#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 313020_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 313020_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 313054_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 313054_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:03:07.03 +01:49:30.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 313055_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 313055_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:52:21.04 -05:34:34.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 3.091 3101891734129376896 103.08775253888 -05.57718780004 13.3163 12.2056 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 313179_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 313179_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 313488_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 313488_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 313548_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 313548_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 313618_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 313618_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 314101_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 314101_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 314250_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 314250_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 314821_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 314821_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:47:09.62 -05:17:18.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 5.126 3100639871420927872 101.78975441255 -05.28971896782 13.7735 12.8711 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.126#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 315110_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 315110_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 315150_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 315150_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 315190_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 315190_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:41:05.38 -05:41:09.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 2.407 3100575683127182848 100.27197276181 -05.68650192790 13.9287 13.3780 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.407#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 315205_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 315205_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:42:15.42 +01:14:35.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 4.737 3125885414305835648 100.56374559839 +01.24197894342 13.9411 13.1211 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.737#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 315209_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 315209_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:52:27.32 -05:52:45.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 2.648 3101108916207784960 103.11340523708 -05.87976646569 14.0840 13.5136 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.648#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 315210_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 315210_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:03:39.53 -00:16:04.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 2.309 3112714776834452352 105.91520285602 -00.26824174127 13.2419 11.2621 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.309#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 315332_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 315332_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 315350_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 315350_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:06:14.87 -04:55:28.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 3.381 3101470827337246464 106.56132619080 -04.92539118273 13.9219 13.2405 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.381#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 315458_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 315458_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 315528_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 315528_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 315599_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 315599_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:56:58.52 -05:23:30.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 3.436 3101205501432136704 104.24419665614 -05.39274442219 14.0641 13.3481 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.436#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 315846_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 315846_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:40:57.05 -04:34:49.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 5.091 3103787734552535808 100.23751504165 -04.58187315124 14.1352 13.3718 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.091#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 315874_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 315874_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 315933_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 315933_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:46:57.54 -02:12:26.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 3.874 3106176389201065728 101.73968461197 -02.20840746904 13.9082 12.8701 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.874#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 316036_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 316036_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 316070_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 316070_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:03:46.87 -01:04:50.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 1.987 3109553199868724224 105.94499944489 -01.08113492279 14.0995 13.5489 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.987#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 316149_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 316149_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 316167_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 316167_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:39:08.71 -03:48:10.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 3.141 3104098655825331328 099.78608026695 -03.80376338268 13.9078 13.3117 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.141#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 316211_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 316211_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 316378_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 316378_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 316470_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 316470_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 316489_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 316489_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 316511_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 316511_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:08:04.50 -01:43:40.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 2.835 3109233104548149120 107.01874958326 -01.72878742697 13.9560 13.4650 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.835#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 316592_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 316592_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 316667_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 316667_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:36:32.37 -03:35:55.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 4.026 3104844850559457792 099.13443358317 -03.59975014338 14.0155 13.4377 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.026#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 316810_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 316810_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:37:09.67 -01:09:02.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 4.592 3118943231029708032 099.29057638008 -01.15179883888 14.0683 13.4931 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.592#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 316927_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 316927_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 317261_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 317261_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 317340_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 317340_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 317390_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 317390_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 317716_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 317716_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 318045_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 318045_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 318084_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 318084_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:52:34.62 +00:32:33.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 5.234 3113580985840503296 103.14371971951 +00.54139619495 14.0748 13.2086 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.234#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 318143_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 318143_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:47:14.64 -03:39:05.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 0.531 3105452708691209216 101.81087051013 -03.65148798860 13.4646 12.2211 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.531#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 318191_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 318191_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:59:45.73 -03:24:18.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 3.854 3102672387384334464 104.94054368107 -03.40607048421 14.1574 13.6542 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.854#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 318323_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 318323_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:06:54.07 +02:10:47.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 318924_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 318924_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:49:54.61 +02:12:16.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 318946_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 318946_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 318972_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 318972_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 318973_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 318973_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 319342_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 319342_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:53:47.95 +00:29:50.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 1.910 3113390186212355840 103.44929652812 +00.49714290746 14.1518 13.6648 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.910#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 319760_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 319760_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 319825_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 319825_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 319982_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 319982_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 319988_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 319988_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 319993_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 319993_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:40:22.44 +01:18:21.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 3.816 3125881084978463744 100.09324944831 +01.30494231969 14.2492 13.7501 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.816#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 320203_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 320203_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 320592_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 320592_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 320636_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 320636_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 320659_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 320659_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 320890_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 320890_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 321064_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 321064_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 321186_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 321186_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 321401_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 321401_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 321406_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 321406_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 321713_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 321713_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:53:27.12 -00:36:02.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 4.248 3112409524919590528 103.36248731965 -00.60181293285 14.0759 13.0152 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.248#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 321723_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 321723_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 321965_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 321965_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:42:59.29 -06:07:27.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 2.720 3100487932657924224 100.74658303668 -06.12485250881 14.3833 13.7807 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.720#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 322206_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 322206_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 322318_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 322318_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:02:48.95 -01:46:38.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 3.623 3109088175171141632 105.70361971433 -01.77817000677 14.4731 14.0617 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.623#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 322327_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 322327_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:37:19.14 +00:16:58.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 3.388 3119703612040020480 099.32944778134 +00.28213637175 12.2889 10.7282 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.388#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 322385_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 322385_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 322597_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 322597_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:49:11.38 -00:25:33.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 3.974 3113216669534339456 102.29729293236 -00.42701368548 14.4407 13.9401 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.974#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 322657_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 322657_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:54:34.31 -01:09:20.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)GAIADR2_OUTPUT=# 2.538 3112325648499548032 103.64279549227 -01.15626921023 14.5400 13.9947 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.538#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 322923_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 322923_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:52:05.43 +00:51:26.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)GAIADR2_OUTPUT=# 3.378 3113605484332811648 103.02252679260 +00.85637243039 14.3468 13.7663 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.378#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 322977_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 322977_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:09:18.42 -05:10:00.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)GAIADR2_OUTPUT=# 3.350 3053365681793813376 107.32624548341 -05.16767196960 14.4569 13.9587 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.350#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 323144_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 323144_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:46:39.58 -05:23:53.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.50, MAG_FAINT_SEARCH_LIMIT=14.48)GAIADR2_OUTPUT=# 2.926 3100637122641982848 101.66459513421 -05.39894167980 13.9070 13.0179 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.926#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 323300_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 323300_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 323397_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 323397_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:00:46.04 -00:47:32.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 5.574 3112623135114648960 105.19109279001 -00.79374862002 14.2400 13.2249 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.574#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 323484_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 323484_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:52:49.28 -00:35:17.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 2.240 3113160903679411200 103.20592279624 -00.58825520483 14.3206 13.2574 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.240#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 323566_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 323566_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 323601_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 323601_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:40:16.38 -03:40:29.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 3.258 3105601967395048704 100.06806845132 -03.67574792297 14.3959 13.4735 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.258#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 323771_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 323771_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:52:24.30 -04:56:14.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 2.604 3102068068304979840 103.10112064737 -04.93798955510 14.5685 13.9898 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.604#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 323860_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 323860_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 323929_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 323929_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:41:02.08 -01:16:58.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.75, MAG_FAINT_SEARCH_LIMIT=14.73)GAIADR2_OUTPUT=# 2.024 3107279925220558336 100.25843447250 -01.28342864787 14.4160 13.4855 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.024#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 323950_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 323950_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 324064_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 324064_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:05:05.57 +00:40:08.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 4.392 3114335147735937408 106.27237447948 +00.66805364881 14.6115 14.2516 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.392#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 324080_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 324080_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:06:38.90 -01:53:09.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 3.644 3109252895757025920 106.66172268544 -01.88689027584 14.4879 13.9728 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.644#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 324157_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 324157_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:39:41.49 +01:00:55.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 3.782 3119862358327569792 099.92284779509 +01.01442208794 14.6637 14.0148 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.782#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 324166_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 324166_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:49:24.42 -01:03:01.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 3.228 3107126508988092544 102.35130968936 -01.05111434072 14.5931 13.8441 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.228#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 324224_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 324224_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:41:53.27 -06:11:56.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.83, MAG_FAINT_SEARCH_LIMIT=14.81)GAIADR2_OUTPUT=# 3.239 3100474704158180864 100.47164385580 -06.19976037553 14.4091 13.8518 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.239#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 324309_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 324309_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:44:18.02 -05:02:41.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 2.355 3100717455709595648 101.07514848917 -05.04548420351 14.7000 14.1919 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.355#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 324383_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 324383_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 324407_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 324407_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:46:39.46 +01:45:17.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 5.107 3125969080270305920 101.66392389435 +01.75355861020 14.4022 13.7868 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.107#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 324473_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 324473_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 324516_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 324516_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:39:40.12 +00:06:19.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 3.810 3119730382573570816 099.91675113215 +00.10455432519 14.8349 14.0195 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.810#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 324533_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 324533_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 324557_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 324557_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:41:17.20 +02:07:59.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 3.628 3126790071859198208 100.32095100740 +02.13245652543 14.8308 14.2333 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.628#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 324589_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 324589_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:07:43.49 -01:54:15.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.75, MAG_FAINT_SEARCH_LIMIT=14.73)GAIADR2_OUTPUT=# 4.474 3109203177216186240 106.93032549396 -01.90518073974 14.6078 14.3396 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.474#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 324596_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 324596_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:39:22.19 -04:11:17.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 3.502 3104000459989380352 099.84229353271 -04.18904210370 14.5055 13.7184 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.502#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 324655_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 324655_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:05:40.12 -05:52:26.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 3.416 3053225322262390656 106.41637127690 -05.87441269746 14.6240 14.2104 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.416#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 324678_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 324678_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:46:15.59 -02:42:19.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 4.617 3105771292185485312 101.56464830605 -02.70657782266 14.7179 14.0601 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.617#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 324800_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 324800_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 324807_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 324807_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:56:43.14 -03:40:08.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)GAIADR2_OUTPUT=# 3.189 3102647270415412352 104.17930650119 -03.66982275912 14.4610 13.9606 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.189#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 324824_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 324824_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:52:56.03 -04:50:51.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 1.987 3102075112051250048 103.23316661724 -04.84816368675 14.7025 14.1051 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.987#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 324842_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 324842_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:03:42.24 -00:35:20.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 0.820 3112599602992583168 105.92611366219 -00.58925302145 14.4325 13.6354 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.820#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 324871_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 324871_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:45:11.04 -03:27:40.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 4.479 3105657458372822784 101.29548014967 -03.46235313718 14.7056 14.1273 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.479#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 324929_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 324929_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 324952_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 324952_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:58:00.26 -01:45:47.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.92, MAG_FAINT_SEARCH_LIMIT=14.90)GAIADR2_OUTPUT=# 5.690 3112037477673436160 104.50146582481 -01.76483931623 14.8766 14.3308 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.690#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 325010_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 325010_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:59:58.69 +00:25:57.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 4.163 3113048409894355712 104.99492860116 +00.43149355412 14.4183 13.6071 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.163#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 325031_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 325031_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:49:37.89 +01:39:28.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 3.016 3126135347044320640 102.40754657834 +01.65720146843 14.7441 14.1556 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.016#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 325035_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 325035_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:51:48.02 -01:14:19.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 1.802 3112359114884221824 102.94983046878 -01.23909881411 14.6899 14.2365 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.802#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 325070_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 325070_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:52:51.76 -03:30:56.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.92, MAG_FAINT_SEARCH_LIMIT=14.90)GAIADR2_OUTPUT=# 4.092 3102785293483602816 103.21521802092 -03.51676705530 14.5044 13.5733 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.092#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 325086_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 325086_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:44:14.56 +01:21:10.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 5.217 3125844182620075520 101.05972488389 +01.35192628519 14.6520 14.1094 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.217#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 325094_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 325094_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 325153_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 325153_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 325157_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
Preparing report for the candidate 325157_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
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Considering the candidate 325261_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 325261_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:59:02.25 -04:28:20.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 3.542 3101704714070295296 104.75905372799 -04.47329144689 14.6947 14.1912 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.542#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 325288_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 325288_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:09:02.16 -02:03:20.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 3.414 3109207953220300928 107.25851995120 -02.05656806448 14.6932 14.1940 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.414#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 325327_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 325327_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:59:37.41 -05:48:38.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 2.439 3100977833808615808 104.90539394993 -05.81122972166 14.5576 13.9153 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.439#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 230048_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 230048_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
Rejecting candidate due to large distance (25.4") between the two second-epoch detections
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Considering the candidate 121122_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 121122_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:09:13.65 -02:21:30.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 199360_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 199360_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 07:08:45.35 +00:41:48.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 124597_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 124597_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
Rejecting candidate due to large distance (23.3") between the two second-epoch detections
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Considering the candidate 154583_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 154583_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:41:59.22 -01:11:07.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31804_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 31804_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:37:53.21 -05:55:17.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 145090_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 145090_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
Rejecting candidate due to large distance (24.8") between the two second-epoch detections
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Considering the candidate 228912_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356
The candidate 228912_fd_Mon-02-Q2b1x1_2026-04-18_21-43-09_20.00sec_-5.00C_LIGHT_0356 did not pass the final checks
**** FOUND 06:50:00.73 +01:46:34.2 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 13s
make_report_in_HTML.sh TOTAL: 567s
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 ####
06:41:52.25 -05:30:57.4
07:04:59.46 -05:12:08.6
06:44:58.53 +00:57:06.9
07:01:14.75 -02:44:16.9
06:56:48.80 +02:10:37.6
06:50:01.35 +01:08:24.2
07:03:29.11 -01:38:50.4
07:07:08.46 -02:45:58.5
06:58:00.70 -02:48:59.5
06:54:06.80 -01:31:49.3
07:03:34.51 -06:11:12.7
06:56:39.28 -02:13:31.3
07:06:56.34 +00:23:24.0
06:54:40.57 -01:56:11.2
06:53:51.71 -01:17:01.5
06:55:07.46 -02:37:23.3
06:53:42.69 -03:34:07.5
06:50:57.40 -01:59:58.3
06:58:43.29 -01:49:10.7
07:03:41.01 -02:10:57.3
06:43:09.64 -02:13:05.6
07:01:12.29 -01:23:36.4
06:47:32.90 +00:59:47.6
06:56:26.14 -02:53:13.1
07:03:36.13 -03:22:58.9
06:47:27.83 -01:05:51.7
06:51:59.94 +00:27:10.5
06:50:00.15 -05:55:19.0
07:02:49.12 -05:28:13.9
06:45:13.11 -00:39:27.0
07:09:51.92 -05:21:54.6
07:07:42.94 -02:06:39.6
07:02:12.49 -04:22:05.5
06:46:46.43 -05:31:23.3
06:43:56.53 -05:38:37.3
06:51:10.19 -02:40:57.4
07:02:23.95 -01:34:38.3
06:53:43.52 -01:58:43.0
06:44:12.33 -00:00:20.9
07:01:43.84 -01:10:42.5
06:53:05.79 -05:33:50.2
06:56:27.65 -01:27:43.3
06:51:11.46 -02:22:09.8
06:59:04.01 -02:15:14.6
07:09:27.13 -00:57:18.6
06:46:32.58 -01:51:13.2
06:56:04.48 -01:29:58.8
07:08:17.19 -04:56:00.7
06:58:39.26 -01:55:23.5
06:45:06.88 -01:17:20.7
07:00:00.11 -05:53:48.8
06:59:01.00 -02:36:03.2
07:02:47.23 -03:51:37.0
07:07:45.99 -03:10:12.5
06:45:26.98 -05:18:36.6
06:53:22.58 -03:34:22.9
07:06:51.81 -05:24:28.3
06:57:07.02 -00:31:51.4
07:03:59.42 -05:30:49.0
06:57:55.61 -01:46:59.6
07:00:09.69 -00:53:34.6
06:44:25.40 +01:06:41.5
06:54:59.11 -05:04:37.5
07:04:05.58 +00:58:05.8
07:03:39.75 -04:38:24.0
07:06:50.26 +00:50:33.6
07:05:05.71 -03:34:37.0
07:06:31.66 +01:08:37.7
07:01:33.73 -00:32:33.4
06:58:09.42 -01:16:02.1
07:09:26.58 -02:33:16.7
06:53:04.48 -05:33:23.6
06:54:41.09 -02:07:02.0
07:02:05.77 -02:46:38.1
07:06:46.66 -01:31:18.2
07:02:57.90 -00:25:26.1
07:03:24.64 -05:00:15.5
07:06:13.29 -03:12:30.5
06:51:52.90 -04:24:14.9
06:38:37.60 -02:21:14.9
06:40:43.61 -01:24:09.5
07:01:15.25 -06:13:20.0
07:08:48.79 -03:42:58.7
07:07:51.47 -05:46:59.9
06:49:52.37 -02:39:52.7
07:09:08.41 -01:41:26.7
07:05:09.83 -06:04:37.2
06:46:13.87 +00:50:43.1
07:09:10.35 -01:30:23.0
06:42:21.50 -05:13:54.2
07:03:25.13 -05:00:40.5
06:51:12.94 -00:35:21.7
07:04:42.38 -04:08:44.8
07:08:32.37 -04:39:28.8
06:53:36.72 -02:31:47.7
07:06:47.91 -03:23:13.7
06:59:30.37 +00:22:08.2
07:07:02.43 -01:57:17.0
06:35:07.42 -03:03:03.8
07:07:43.10 -02:39:44.4
06:44:34.05 -01:35:29.2
07:06:42.33 -03:09:11.6
06:58:57.09 -03:00:41.1
07:05:50.92 -02:05:13.3
07:02:21.42 -04:03:31.4
06:44:24.58 +01:58:58.7
06:45:12.35 -00:01:51.7
06:50:14.48 -00:47:12.5
06:50:47.02 -05:49:03.5
07:06:17.15 +02:00:15.1
06:48:50.55 -00:08:31.6
07:09:03.27 -02:29:04.9
06:51:05.03 -01:41:33.8
07:03:52.66 -06:00:23.9
07:08:43.28 -05:05:29.4
06:52:55.15 -02:23:02.7
06:54:23.36 -01:37:01.2
06:56:22.04 -00:53:11.9
06:43:47.08 +01:14:20.3
06:54:48.38 +00:23:18.5
07:03:04.46 -01:18:38.1
06:49:56.14 -02:40:55.2
06:47:10.33 -05:37:12.4
06:58:50.15 -04:41:11.0
06:48:53.17 +01:49:30.1
06:57:24.11 -02:57:03.7
06:58:00.35 -00:22:01.1
06:58:35.47 -04:20:28.6
06:57:12.43 -03:57:45.8
07:04:16.84 -03:01:38.5
06:42:33.16 -03:28:07.1
06:49:07.29 -01:40:16.8
06:43:36.92 -04:25:01.8
07:04:56.01 -05:21:46.4
06:41:27.03 -01:19:01.3
06:43:55.46 -05:04:01.2
06:51:34.31 -01:39:23.4
06:46:10.30 -03:13:58.6
06:42:30.96 -06:04:21.5
06:44:50.61 +01:05:43.9
06:40:05.93 +00:25:10.5
06:49:56.03 -02:17:02.2
06:54:17.81 -04:54:48.1
06:37:27.04 -02:40:39.0
06:47:14.98 -05:48:24.9
06:45:17.59 +00:43:39.8
07:08:59.14 -00:34:33.0
06:38:58.51 -00:30:12.9
06:44:57.65 -02:51:41.3
06:53:41.39 -00:33:48.9
06:57:35.71 +01:13:53.0
06:35:21.82 -05:17:32.3
06:51:23.95 +00:52:43.8
06:38:41.66 +01:56:40.1
06:40:45.50 -03:54:51.5
06:38:49.83 +02:05:40.8
06:57:27.82 -05:05:44.2
06:41:21.16 -01:43:20.4
07:05:25.41 -03:18:31.6
06:49:24.55 -00:56:17.3
06:54:22.80 -02:36:36.2
06:37:07.38 -01:00:19.4
06:48:34.64 -03:13:29.6
06:55:50.64 -02:12:28.8
06:55:26.35 -02:12:44.7
06:40:50.58 +00:57:15.6
06:38:39.70 +01:56:44.2
06:51:35.01 -02:45:18.3
07:01:56.11 +01:13:07.8
06:58:34.68 -01:38:22.5
06:44:38.28 -02:01:19.3
06:51:17.94 -01:57:55.9
06:57:16.55 -02:44:41.9
06:58:20.38 -00:32:37.9
06:52:50.97 -02:20:52.3
06:40:57.51 -03:41:09.2
06:55:37.71 -05:35:29.8
07:09:14.02 -03:42:55.6
06:42:59.47 +00:50:06.0
07:03:54.03 -00:56:59.2
07:02:35.21 -06:06:06.7
06:51:43.41 -01:38:55.8
06:48:43.87 -05:54:26.4
06:51:36.63 -02:04:10.2
06:41:46.37 -00:57:08.2
06:47:04.30 +01:23:25.1
06:43:24.65 -00:26:07.7
06:42:36.24 +00:14:26.2
07:03:41.07 -04:17:23.5
06:54:53.44 -01:04:23.5
06:53:48.85 -03:17:34.4
07:02:38.29 -04:51:08.1
06:57:43.47 -02:07:57.6
06:51:09.62 +00:53:03.1
06:49:16.80 -00:21:50.7
06:52:01.72 -00:36:53.6
06:57:39.38 -03:34:43.4
06:53:09.49 -01:41:54.9
06:54:03.07 -00:10:55.1
########### 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 ####
06:41:52.25 -05:30:57.4
07:04:59.46 -05:12:08.6
06:44:58.53 +00:57:06.9
07:01:14.75 -02:44:16.9
06:56:48.80 +02:10:37.6
06:50:01.35 +01:08:24.2
07:03:29.11 -01:38:50.4
07:07:08.46 -02:45:58.5
06:58:00.70 -02:48:59.5
06:54:06.80 -01:31:49.3
07:03:34.51 -06:11:12.7
06:56:39.28 -02:13:31.3
07:06:56.34 +00:23:24.0
06:54:40.57 -01:56:11.2
06:53:51.71 -01:17:01.5
06:55:07.46 -02:37:23.3
06:53:42.69 -03:34:07.5
06:50:57.40 -01:59:58.3
06:58:43.29 -01:49:10.7
07:03:41.01 -02:10:57.3
06:43:09.64 -02:13:05.6
07:01:12.29 -01:23:36.4
06:47:32.90 +00:59:47.6
06:56:26.14 -02:53:13.1
07:03:36.13 -03:22:58.9
06:47:27.83 -01:05:51.7
06:51:59.94 +00:27:10.5
06:50:00.15 -05:55:19.0
07:02:49.12 -05:28:13.9
06:45:13.11 -00:39:27.0
07:09:51.92 -05:21:54.6
07:07:42.94 -02:06:39.6
07:02:12.49 -04:22:05.5
06:46:46.43 -05:31:23.3
06:43:56.53 -05:38:37.3
06:51:10.19 -02:40:57.4
07:02:23.95 -01:34:38.3
06:53:43.52 -01:58:43.0
06:44:12.33 -00:00:20.9
07:01:43.84 -01:10:42.5
06:53:05.79 -05:33:50.2
06:56:27.65 -01:27:43.3
06:51:11.46 -02:22:09.8
06:59:04.01 -02:15:14.6
07:09:27.13 -00:57:18.6
06:46:32.58 -01:51:13.2
06:56:04.48 -01:29:58.8
07:08:17.19 -04:56:00.7
06:58:39.26 -01:55:23.5
06:45:06.88 -01:17:20.7
07:00:00.11 -05:53:48.8
06:59:01.00 -02:36:03.2
07:02:47.23 -03:51:37.0
07:07:45.99 -03:10:12.5
06:45:26.98 -05:18:36.6
06:53:22.58 -03:34:22.9
07:06:51.81 -05:24:28.3
06:57:07.02 -00:31:51.4
07:03:59.42 -05:30:49.0
06:57:55.61 -01:46:59.6
07:00:09.69 -00:53:34.6
06:44:25.40 +01:06:41.5
06:54:59.11 -05:04:37.5
07:04:05.58 +00:58:05.8
07:03:39.75 -04:38:24.0
07:06:50.26 +00:50:33.6
07:05:05.71 -03:34:37.0
07:06:31.66 +01:08:37.7
07:01:33.73 -00:32:33.4
06:58:09.42 -01:16:02.1
07:09:26.58 -02:33:16.7
06:53:04.48 -05:33:23.6
06:54:41.09 -02:07:02.0
07:02:05.77 -02:46:38.1
07:06:46.66 -01:31:18.2
07:02:57.90 -00:25:26.1
07:03:24.64 -05:00:15.5
07:06:13.29 -03:12:30.5
06:51:52.90 -04:24:14.9
06:38:37.60 -02:21:14.9
06:40:43.61 -01:24:09.5
07:01:15.25 -06:13:20.0
07:08:48.79 -03:42:58.7
07:07:51.47 -05:46:59.9
06:49:52.37 -02:39:52.7
07:09:08.41 -01:41:26.7
07:05:09.83 -06:04:37.2
06:46:13.87 +00:50:43.1
07:09:10.35 -01:30:23.0
06:42:21.50 -05:13:54.2
07:03:25.13 -05:00:40.5
06:51:12.94 -00:35:21.7
07:04:42.38 -04:08:44.8
07:08:32.37 -04:39:28.8
06:53:36.72 -02:31:47.7
07:06:47.91 -03:23:13.7
06:59:30.37 +00:22:08.2
07:07:02.43 -01:57:17.0
06:35:07.42 -03:03:03.8
07:07:43.10 -02:39:44.4
06:44:34.05 -01:35:29.2
07:06:42.33 -03:09:11.6
06:58:57.09 -03:00:41.1
07:05:50.92 -02:05:13.3
07:02:21.42 -04:03:31.4
06:44:24.58 +01:58:58.7
06:45:12.35 -00:01:51.7
06:50:14.48 -00:47:12.5
06:50:47.02 -05:49:03.5
07:06:17.15 +02:00:15.1
06:48:50.55 -00:08:31.6
07:09:03.27 -02:29:04.9
06:51:05.03 -01:41:33.8
07:03:52.66 -06:00:23.9
07:08:43.28 -05:05:29.4
06:52:55.15 -02:23:02.7
06:54:23.36 -01:37:01.2
06:56:22.04 -00:53:11.9
06:43:47.08 +01:14:20.3
06:54:48.38 +00:23:18.5
07:03:04.46 -01:18:38.1
06:49:56.14 -02:40:55.2
06:47:10.33 -05:37:12.4
06:58:50.15 -04:41:11.0
06:48:53.17 +01:49:30.1
06:57:24.11 -02:57:03.7
06:58:00.35 -00:22:01.1
06:58:35.47 -04:20:28.6
06:57:12.43 -03:57:45.8
07:04:16.84 -03:01:38.5
06:42:33.16 -03:28:07.1
06:49:07.29 -01:40:16.8
06:43:36.92 -04:25:01.8
07:04:56.01 -05:21:46.4
06:41:27.03 -01:19:01.3
06:43:55.46 -05:04:01.2
06:51:34.31 -01:39:23.4
06:46:10.30 -03:13:58.6
06:42:30.96 -06:04:21.5
06:44:50.61 +01:05:43.9
06:40:05.93 +00:25:10.5
06:49:56.03 -02:17:02.2
06:54:17.81 -04:54:48.1
06:37:27.04 -02:40:39.0
06:47:14.98 -05:48:24.9
06:45:17.59 +00:43:39.8
07:08:59.14 -00:34:33.0
06:38:58.51 -00:30:12.9
06:44:57.65 -02:51:41.3
06:53:41.39 -00:33:48.9
06:57:35.71 +01:13:53.0
06:35:21.82 -05:17:32.3
06:51:23.95 +00:52:43.8
06:38:41.66 +01:56:40.1
06:40:45.50 -03:54:51.5
06:38:49.83 +02:05:40.8
06:57:27.82 -05:05:44.2
06:41:21.16 -01:43:20.4
07:05:25.41 -03:18:31.6
06:49:24.55 -00:56:17.3
06:54:22.80 -02:36:36.2
06:37:07.38 -01:00:19.4
06:48:34.64 -03:13:29.6
06:55:50.64 -02:12:28.8
06:55:26.35 -02:12:44.7
06:40:50.58 +00:57:15.6
06:38:39.70 +01:56:44.2
06:51:35.01 -02:45:18.3
07:01:56.11 +01:13:07.8
06:58:34.68 -01:38:22.5
06:44:38.28 -02:01:19.3
06:51:17.94 -01:57:55.9
06:57:16.55 -02:44:41.9
06:58:20.38 -00:32:37.9
06:52:50.97 -02:20:52.3
06:40:57.51 -03:41:09.2
06:55:37.71 -05:35:29.8
07:09:14.02 -03:42:55.6
06:42:59.47 +00:50:06.0
07:03:54.03 -00:56:59.2
07:02:35.21 -06:06:06.7
06:51:43.41 -01:38:55.8
06:48:43.87 -05:54:26.4
06:51:36.63 -02:04:10.2
06:41:46.37 -00:57:08.2
06:47:04.30 +01:23:25.1
06:43:24.65 -00:26:07.7
06:42:36.24 +00:14:26.2
07:03:41.07 -04:17:23.5
06:54:53.44 -01:04:23.5
06:53:48.85 -03:17:34.4
07:02:38.29 -04:51:08.1
06:57:43.47 -02:07:57.6
06:51:09.62 +00:53:03.1
06:49:16.80 -00:21:50.7
06:52:01.72 -00:36:53.6
06:57:39.38 -03:34:43.4
06:53:09.49 -01:41:54.9
06:54:03.07 -00:10:55.1
###################################################################################
06:41:52.25 -05:30:57.4 -- not an asteroid (will add it to exclusion list)
07:04:59.46 -05:12:08.6 -- not an asteroid (will add it to exclusion list)
06:44:58.53 +00:57:06.9 -- not an asteroid (will add it to exclusion list)
07:01:14.75 -02:44:16.9 -- not an asteroid (will add it to exclusion list)
06:56:48.80 +02:10:37.6 -- not an asteroid (will add it to exclusion list)
06:50:01.35 +01:08:24.2 -- not an asteroid (will add it to exclusion list)
07:03:29.11 -01:38:50.4 -- not an asteroid (will add it to exclusion list)
07:07:08.46 -02:45:58.5 -- not an asteroid (will add it to exclusion list)
06:58:00.70 -02:48:59.5 -- not an asteroid (will add it to exclusion list)
06:54:06.80 -01:31:49.3 -- not an asteroid (will add it to exclusion list)
07:03:34.51 -06:11:12.7 -- not an asteroid (will add it to exclusion list)
06:56:39.28 -02:13:31.3 -- not an asteroid (will add it to exclusion list)
07:06:56.34 +00:23:24.0 -- not an asteroid (will add it to exclusion list)
06:54:40.57 -01:56:11.2 -- not an asteroid (will add it to exclusion list)
06:53:51.71 -01:17:01.5 -- not an asteroid (will add it to exclusion list)
06:55:07.46 -02:37:23.3 -- not an asteroid (will add it to exclusion list)
06:53:42.69 -03:34:07.5 -- not an asteroid (will add it to exclusion list)
06:50:57.40 -01:59:58.3 -- not an asteroid (will add it to exclusion list)
06:58:43.29 -01:49:10.7 -- not an asteroid (will add it to exclusion list)
07:03:41.01 -02:10:57.3 -- not an asteroid (will add it to exclusion list)
06:43:09.64 -02:13:05.6 -- not an asteroid (will add it to exclusion list)
07:01:12.29 -01:23:36.4 -- not an asteroid (will add it to exclusion list)
06:47:32.90 +00:59:47.6 -- not an asteroid (will add it to exclusion list)
06:56:26.14 -02:53:13.1 -- not an asteroid (will add it to exclusion list)
07:03:36.13 -03:22:58.9 -- not an asteroid (will add it to exclusion list)
06:47:27.83 -01:05:51.7 -- not an asteroid (will add it to exclusion list)
06:51:59.94 +00:27:10.5 -- not an asteroid (will add it to exclusion list)
06:50:00.15 -05:55:19.0 -- not an asteroid (will add it to exclusion list)
07:02:49.12 -05:28:13.9 -- not an asteroid (will add it to exclusion list)
06:45:13.11 -00:39:27.0 -- not an asteroid (will add it to exclusion list)
07:09:51.92 -05:21:54.6 -- not an asteroid (will add it to exclusion list)
07:07:42.94 -02:06:39.6 -- not an asteroid (will add it to exclusion list)
07:02:12.49 -04:22:05.5 -- not an asteroid (will add it to exclusion list)
06:46:46.43 -05:31:23.3 -- not an asteroid (will add it to exclusion list)
06:43:56.53 -05:38:37.3 -- not an asteroid (will add it to exclusion list)
06:51:10.19 -02:40:57.4 -- not an asteroid (will add it to exclusion list)
07:02:23.95 -01:34:38.3 -- not an asteroid (will add it to exclusion list)
06:53:43.52 -01:58:43.0 -- not an asteroid (will add it to exclusion list)
06:44:12.33 -00:00:20.9 -- not an asteroid (will add it to exclusion list)
07:01:43.84 -01:10:42.5 -- not an asteroid (will add it to exclusion list)
06:53:05.79 -05:33:50.2 -- not an asteroid (will add it to exclusion list)
06:56:27.65 -01:27:43.3 -- not an asteroid (will add it to exclusion list)
06:51:11.46 -02:22:09.8 -- not an asteroid (will add it to exclusion list)
06:59:04.01 -02:15:14.6 -- not an asteroid (will add it to exclusion list)
07:09:27.13 -00:57:18.6 -- not an asteroid (will add it to exclusion list)
06:46:32.58 -01:51:13.2 -- not an asteroid (will add it to exclusion list)
06:56:04.48 -01:29:58.8 -- not an asteroid (will add it to exclusion list)
07:08:17.19 -04:56:00.7 -- not an asteroid (will add it to exclusion list)
06:58:39.26 -01:55:23.5 -- not an asteroid (will add it to exclusion list)
06:45:06.88 -01:17:20.7 -- not an asteroid (will add it to exclusion list)
07:00:00.11 -05:53:48.8 -- not an asteroid (will add it to exclusion list)
06:59:01.00 -02:36:03.2 -- not an asteroid (will add it to exclusion list)
07:02:47.23 -03:51:37.0 -- not an asteroid (will add it to exclusion list)
07:07:45.99 -03:10:12.5 -- not an asteroid (will add it to exclusion list)
06:45:26.98 -05:18:36.6 -- not an asteroid (will add it to exclusion list)
06:53:22.58 -03:34:22.9 -- not an asteroid (will add it to exclusion list)
07:06:51.81 -05:24:28.3 -- not an asteroid (will add it to exclusion list)
06:57:07.02 -00:31:51.4 -- not an asteroid (will add it to exclusion list)
07:03:59.42 -05:30:49.0 -- not an asteroid (will add it to exclusion list)
06:57:55.61 -01:46:59.6 -- not an asteroid (will add it to exclusion list)
07:00:09.69 -00:53:34.6 -- not an asteroid (will add it to exclusion list)
06:44:25.40 +01:06:41.5 -- not an asteroid (will add it to exclusion list)
06:54:59.11 -05:04:37.5 -- not an asteroid (will add it to exclusion list)
07:04:05.58 +00:58:05.8 -- not an asteroid (will add it to exclusion list)
07:03:39.75 -04:38:24.0 -- not an asteroid (will add it to exclusion list)
07:06:50.26 +00:50:33.6 -- not an asteroid (will add it to exclusion list)
07:05:05.71 -03:34:37.0 -- not an asteroid (will add it to exclusion list)
07:06:31.66 +01:08:37.7 -- not an asteroid (will add it to exclusion list)
07:01:33.73 -00:32:33.4 -- not an asteroid (will add it to exclusion list)
06:58:09.42 -01:16:02.1 -- not an asteroid (will add it to exclusion list)
07:09:26.58 -02:33:16.7 -- not an asteroid (will add it to exclusion list)
06:53:04.48 -05:33:23.6 -- not an asteroid (will add it to exclusion list)
06:54:41.09 -02:07:02.0 -- not an asteroid (will add it to exclusion list)
07:02:05.77 -02:46:38.1 -- not an asteroid (will add it to exclusion list)
07:06:46.66 -01:31:18.2 -- not an asteroid (will add it to exclusion list)
07:02:57.90 -00:25:26.1 -- not an asteroid (will add it to exclusion list)
07:03:24.64 -05:00:15.5 -- not an asteroid (will add it to exclusion list)
07:06:13.29 -03:12:30.5 -- not an asteroid (will add it to exclusion list)
06:51:52.90 -04:24:14.9 -- not an asteroid (will add it to exclusion list)
06:38:37.60 -02:21:14.9 -- not an asteroid (will add it to exclusion list)
06:40:43.61 -01:24:09.5 -- not an asteroid (will add it to exclusion list)
07:01:15.25 -06:13:20.0 -- not an asteroid (will add it to exclusion list)
07:08:48.79 -03:42:58.7 -- not an asteroid (will add it to exclusion list)
07:07:51.47 -05:46:59.9 -- not an asteroid (will add it to exclusion list)
06:49:52.37 -02:39:52.7 -- not an asteroid (will add it to exclusion list)
07:09:08.41 -01:41:26.7 -- not an asteroid (will add it to exclusion list)
07:05:09.83 -06:04:37.2 -- not an asteroid (will add it to exclusion list)
06:46:13.87 +00:50:43.1 -- not an asteroid (will add it to exclusion list)
07:09:10.35 -01:30:23.0 -- not an asteroid (will add it to exclusion list)
06:42:21.50 -05:13:54.2 -- not an asteroid (will add it to exclusion list)
07:03:25.13 -05:00:40.5 -- not an asteroid (will add it to exclusion list)
06:51:12.94 -00:35:21.7 -- not an asteroid (will add it to exclusion list)
07:04:42.38 -04:08:44.8 -- not an asteroid (will add it to exclusion list)
07:08:32.37 -04:39:28.8 -- not an asteroid (will add it to exclusion list)
06:53:36.72 -02:31:47.7 -- not an asteroid (will add it to exclusion list)
07:06:47.91 -03:23:13.7 -- not an asteroid (will add it to exclusion list)
06:59:30.37 +00:22:08.2 -- not an asteroid (will add it to exclusion list)
07:07:02.43 -01:57:17.0 -- not an asteroid (will add it to exclusion list)
06:35:07.42 -03:03:03.8 -- not an asteroid (will add it to exclusion list)
07:07:43.10 -02:39:44.4 -- not an asteroid (will add it to exclusion list)
06:44:34.05 -01:35:29.2 -- not an asteroid (will add it to exclusion list)
07:06:42.33 -03:09:11.6 -- not an asteroid (will add it to exclusion list)
06:58:57.09 -03:00:41.1 -- not an asteroid (will add it to exclusion list)
07:05:50.92 -02:05:13.3 -- not an asteroid (will add it to exclusion list)
07:02:21.42 -04:03:31.4 -- not an asteroid (will add it to exclusion list)
06:44:24.58 +01:58:58.7 -- not an asteroid (will add it to exclusion list)
06:45:12.35 -00:01:51.7 -- not an asteroid (will add it to exclusion list)
06:50:14.48 -00:47:12.5 -- not an asteroid (will add it to exclusion list)
06:50:47.02 -05:49:03.5 -- not an asteroid (will add it to exclusion list)
07:06:17.15 +02:00:15.1 -- not an asteroid (will add it to exclusion list)
06:48:50.55 -00:08:31.6 -- not an asteroid (will add it to exclusion list)
07:09:03.27 -02:29:04.9 -- not an asteroid (will add it to exclusion list)
06:51:05.03 -01:41:33.8 -- not an asteroid (will add it to exclusion list)
07:03:52.66 -06:00:23.9 -- not an asteroid (will add it to exclusion list)
07:08:43.28 -05:05:29.4 -- not an asteroid (will add it to exclusion list)
06:52:55.15 -02:23:02.7 -- not an asteroid (will add it to exclusion list)
06:54:23.36 -01:37:01.2 -- not an asteroid (will add it to exclusion list)
06:56:22.04 -00:53:11.9 -- not an asteroid (will add it to exclusion list)
06:43:47.08 +01:14:20.3 -- not an asteroid (will add it to exclusion list)
06:54:48.38 +00:23:18.5 -- not an asteroid (will add it to exclusion list)
07:03:04.46 -01:18:38.1 -- not an asteroid (will add it to exclusion list)
06:49:56.14 -02:40:55.2 -- not an asteroid (will add it to exclusion list)
06:47:10.33 -05:37:12.4 -- not an asteroid (will add it to exclusion list)
06:58:50.15 -04:41:11.0 -- not an asteroid (will add it to exclusion list)
06:48:53.17 +01:49:30.1 -- not an asteroid (will add it to exclusion list)
06:57:24.11 -02:57:03.7 -- not an asteroid (will add it to exclusion list)
06:58:00.35 -00:22:01.1 -- not an asteroid (will add it to exclusion list)
06:58:35.47 -04:20:28.6 -- not an asteroid (will add it to exclusion list)
06:57:12.43 -03:57:45.8 -- not an asteroid (will add it to exclusion list)
07:04:16.84 -03:01:38.5 -- not an asteroid (will add it to exclusion list)
06:42:33.16 -03:28:07.1 -- not an asteroid (will add it to exclusion list)
06:49:07.29 -01:40:16.8 -- not an asteroid (will add it to exclusion list)
06:43:36.92 -04:25:01.8 -- not an asteroid (will add it to exclusion list)
07:04:56.01 -05:21:46.4 -- not an asteroid (will add it to exclusion list)
06:41:27.03 -01:19:01.3 -- not an asteroid (will add it to exclusion list)
06:43:55.46 -05:04:01.2 -- not an asteroid (will add it to exclusion list)
06:51:34.31 -01:39:23.4 -- not an asteroid (will add it to exclusion list)
06:46:10.30 -03:13:58.6 -- not an asteroid (will add it to exclusion list)
06:42:30.96 -06:04:21.5 -- not an asteroid (will add it to exclusion list)
06:44:50.61 +01:05:43.9 -- not an asteroid (will add it to exclusion list)
06:40:05.93 +00:25:10.5 -- not an asteroid (will add it to exclusion list)
06:49:56.03 -02:17:02.2 -- not an asteroid (will add it to exclusion list)
06:54:17.81 -04:54:48.1 -- not an asteroid (will add it to exclusion list)
06:37:27.04 -02:40:39.0 -- not an asteroid (will add it to exclusion list)
06:47:14.98 -05:48:24.9 -- not an asteroid (will add it to exclusion list)
06:45:17.59 +00:43:39.8 -- not an asteroid (will add it to exclusion list)
07:08:59.14 -00:34:33.0 -- not an asteroid (will add it to exclusion list)
06:38:58.51 -00:30:12.9 -- not an asteroid (will add it to exclusion list)
06:44:57.65 -02:51:41.3 -- not an asteroid (will add it to exclusion list)
06:53:41.39 -00:33:48.9 -- not an asteroid (will add it to exclusion list)
06:57:35.71 +01:13:53.0 -- not an asteroid (will add it to exclusion list)
06:35:21.82 -05:17:32.3 -- not an asteroid (will add it to exclusion list)
06:51:23.95 +00:52:43.8 -- not an asteroid (will add it to exclusion list)
06:38:41.66 +01:56:40.1 -- not an asteroid (will add it to exclusion list)
06:40:45.50 -03:54:51.5 -- not an asteroid (will add it to exclusion list)
06:38:49.83 +02:05:40.8 -- not an asteroid (will add it to exclusion list)
06:57:27.82 -05:05:44.2 -- not an asteroid (will add it to exclusion list)
06:41:21.16 -01:43:20.4 -- not an asteroid (will add it to exclusion list)
07:05:25.41 -03:18:31.6 -- not an asteroid (will add it to exclusion list)
06:49:24.55 -00:56:17.3 -- not an asteroid (will add it to exclusion list)
06:54:22.80 -02:36:36.2 -- not an asteroid (will add it to exclusion list)
06:37:07.38 -01:00:19.4 -- not an asteroid (will add it to exclusion list)
06:48:34.64 -03:13:29.6 -- not an asteroid (will add it to exclusion list)
06:55:50.64 -02:12:28.8 -- not an asteroid (will add it to exclusion list)
06:55:26.35 -02:12:44.7 -- not an asteroid (will add it to exclusion list)
06:40:50.58 +00:57:15.6 -- not an asteroid (will add it to exclusion list)
06:38:39.70 +01:56:44.2 -- not an asteroid (will add it to exclusion list)
06:51:35.01 -02:45:18.3 -- not an asteroid (will add it to exclusion list)
07:01:56.11 +01:13:07.8 -- not an asteroid (will add it to exclusion list)
06:58:34.68 -01:38:22.5 -- not an asteroid (will add it to exclusion list)
06:44:38.28 -02:01:19.3 -- not an asteroid (will add it to exclusion list)
06:51:17.94 -01:57:55.9 -- not an asteroid (will add it to exclusion list)
06:57:16.55 -02:44:41.9 -- not an asteroid (will add it to exclusion list)
06:58:20.38 -00:32:37.9 -- not an asteroid (will add it to exclusion list)
06:52:50.97 -02:20:52.3 -- not an asteroid (will add it to exclusion list)
06:40:57.51 -03:41:09.2 -- not an asteroid (will add it to exclusion list)
06:55:37.71 -05:35:29.8 -- not an asteroid (will add it to exclusion list)
07:09:14.02 -03:42:55.6 -- not an asteroid (will add it to exclusion list)
06:42:59.47 +00:50:06.0 -- not an asteroid (will add it to exclusion list)
07:03:54.03 -00:56:59.2 -- not an asteroid (will add it to exclusion list)
07:02:35.21 -06:06:06.7 -- not an asteroid (will add it to exclusion list)
06:51:43.41 -01:38:55.8 -- not an asteroid (will add it to exclusion list)
06:48:43.87 -05:54:26.4 -- not an asteroid (will add it to exclusion list)
06:51:36.63 -02:04:10.2 -- not an asteroid (will add it to exclusion list)
06:41:46.37 -00:57:08.2 -- not an asteroid (will add it to exclusion list)
06:47:04.30 +01:23:25.1 -- not an asteroid (will add it to exclusion list)
06:43:24.65 -00:26:07.7 -- not an asteroid (will add it to exclusion list)
06:42:36.24 +00:14:26.2 -- not an asteroid (will add it to exclusion list)
07:03:41.07 -04:17:23.5 -- not an asteroid (will add it to exclusion list)
06:54:53.44 -01:04:23.5 -- not an asteroid (will add it to exclusion list)
06:53:48.85 -03:17:34.4 -- not an asteroid (will add it to exclusion list)
07:02:38.29 -04:51:08.1 -- not an asteroid (will add it to exclusion list)
06:57:43.47 -02:07:57.6 -- not an asteroid (will add it to exclusion list)
06:51:09.62 +00:53:03.1 -- not an asteroid (will add it to exclusion list)
06:49:16.80 -00:21:50.7 -- not an asteroid (will add it to exclusion list)
06:52:01.72 -00:36:53.6 -- not an asteroid (will add it to exclusion list)
06:57:39.38 -03:34:43.4 -- not an asteroid (will add it to exclusion list)
06:53:09.49 -01:41:54.9 -- not an asteroid (will add it to exclusion list)
06:54:03.07 -00:10:55.1 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
06:35:07.42 -03:03:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:35:21.82 -05:17:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:37:07.38 -01:00:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:37:27.04 -02:40:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:38:37.60 -02:21:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:38:39.70 +01:56:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:38:41.66 +01:56:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:38:49.83 +02:05:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:38:58.51 -00:30:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:05.93 +00:25:10.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:43.61 -01:24:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:45.50 -03:54:51.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:50.58 +00:57:15.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:40:57.51 -03:41:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:21.16 -01:43:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:27.03 -01:19:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:46.37 -00:57:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:41:52.25 -05:30:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:21.50 -05:13:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:30.96 -06:04:21.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:33.16 -03:28:07.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:36.24 +00:14:26.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:42:59.47 +00:50:06.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:09.64 -02:13:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:24.65 -00:26:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:36.92 -04:25:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:47.08 +01:14:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:55.46 -05:04:01.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:43:56.53 -05:38:37.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:12.33 -00:00:20.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:24.58 +01:58:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:25.40 +01:06:41.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:34.05 -01:35:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:38.28 -02:01:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:50.61 +01:05:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:57.65 -02:51:41.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:44:58.53 +00:57:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:06.88 -01:17:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:12.35 -00:01:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:13.11 -00:39:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:17.59 +00:43:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:45:26.98 -05:18:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:10.30 -03:13:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:13.87 +00:50:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:32.58 -01:51:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:46:46.43 -05:31:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:04.30 +01:23:25.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:10.33 -05:37:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:14.98 -05:48:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:27.83 -01:05:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:47:32.90 +00:59:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:34.64 -03:13:29.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:43.87 -05:54:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:50.55 -00:08:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:48:53.17 +01:49:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:07.29 -01:40:16.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:16.80 -00:21:50.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:24.55 -00:56:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:52.37 -02:39:52.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:56.03 -02:17:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:49:56.14 -02:40:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:00.15 -05:55:19.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:01.35 +01:08:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:14.48 -00:47:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:47.02 -05:49:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:50:57.40 -01:59:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:05.03 -01:41:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:09.62 +00:53:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:10.19 -02:40:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:11.46 -02:22:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:12.94 -00:35:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:17.94 -01:57:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:23.95 +00:52:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:34.31 -01:39:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:35.01 -02:45:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:36.63 -02:04:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:43.41 -01:38:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:52.90 -04:24:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:51:59.94 +00:27:10.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:01.72 -00:36:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:50.97 -02:20:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:52:55.15 -02:23:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:04.48 -05:33:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:05.79 -05:33:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:09.49 -01:41:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:22.58 -03:34:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:36.72 -02:31:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:41.39 -00:33:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:42.69 -03:34:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:43.52 -01:58:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:48.85 -03:17:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:53:51.71 -01:17:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:03.07 -00:10:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:06.80 -01:31:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:17.81 -04:54:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:22.80 -02:36:36.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:23.36 -01:37:01.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:40.57 -01:56:11.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:41.09 -02:07:02.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:48.38 +00:23:18.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:53.44 -01:04:23.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:54:59.11 -05:04:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:07.46 -02:37:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:26.35 -02:12:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:37.71 -05:35:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:55:50.64 -02:12:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:04.48 -01:29:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:22.04 -00:53:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:26.14 -02:53:13.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:27.65 -01:27:43.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:39.28 -02:13:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:56:48.80 +02:10:37.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:07.02 -00:31:51.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:12.43 -03:57:45.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:16.55 -02:44:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:24.11 -02:57:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:27.82 -05:05:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:35.71 +01:13:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:39.38 -03:34:43.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:43.47 -02:07:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:55.61 -01:46:59.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:00.35 -00:22:01.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:00.70 -02:48:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:09.42 -01:16:02.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:20.38 -00:32:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:34.68 -01:38:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:35.47 -04:20:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:39.26 -01:55:23.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:43.29 -01:49:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:50.15 -04:41:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:57.09 -03:00:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:01.00 -02:36:03.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:04.01 -02:15:14.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:30.37 +00:22:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:00.11 -05:53:48.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:09.69 -00:53:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:12.29 -01:23:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:14.75 -02:44:16.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:15.25 -06:13:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:33.73 -00:32:33.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:43.84 -01:10:42.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:56.11 +01:13:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:05.77 -02:46:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:12.49 -04:22:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:21.42 -04:03:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:23.95 -01:34:38.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:35.21 -06:06:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:38.29 -04:51:08.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:47.23 -03:51:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:49.12 -05:28:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:57.90 -00:25:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:04.46 -01:18:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:24.64 -05:00:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:25.13 -05:00:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:29.11 -01:38:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:34.51 -06:11:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:36.13 -03:22:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:39.75 -04:38:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:41.01 -02:10:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:41.07 -04:17:23.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:52.66 -06:00:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:54.03 -00:56:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:03:59.42 -05:30:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:05.58 +00:58:05.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:16.84 -03:01:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:42.38 -04:08:44.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:56.01 -05:21:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:59.46 -05:12:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:05.71 -03:34:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:09.83 -06:04:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:25.41 -03:18:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:05:50.92 -02:05:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:13.29 -03:12:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:17.15 +02:00:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:31.66 +01:08:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:42.33 -03:09:11.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:46.66 -01:31:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:47.91 -03:23:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:50.26 +00:50:33.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:51.81 -05:24:28.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:06:56.34 +00:23:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:02.43 -01:57:17.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:08.46 -02:45:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:42.94 -02:06:39.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:43.10 -02:39:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:45.99 -03:10:12.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:07:51.47 -05:46:59.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:17.19 -04:56:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:32.37 -04:39:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:43.28 -05:05:29.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:48.79 -03:42:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:08:59.14 -00:34:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:03.27 -02:29:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:08.41 -01:41:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:10.35 -01:30:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:14.02 -03:42:55.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:26.58 -02:33:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:27.13 -00:57:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:09:51.92 -05:21:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
06:35:07.42 -03:03:03.8 -- not a known variable star
06:35:21.82 -05:17:32.3 -- not a known variable star
06:37:07.38 -01:00:19.4 -- not a known variable star
06:37:27.04 -02:40:39.0 -- not a known variable star
06:38:37.60 -02:21:14.9 -- not a known variable star
06:38:39.70 +01:56:44.2 -- not a known variable star
06:38:41.66 +01:56:40.1 -- not a known variable star
06:38:49.83 +02:05:40.8 -- a known variable star
06:38:58.51 -00:30:12.9 -- not a known variable star
06:40:05.93 +00:25:10.5 -- not a known variable star
06:40:43.61 -01:24:09.5 -- a known variable star
06:40:45.50 -03:54:51.5 -- not a known variable star
06:40:50.58 +00:57:15.6 -- not a known variable star
06:40:57.51 -03:41:09.2 -- not a known variable star
06:41:21.16 -01:43:20.4 -- not a known variable star
06:41:27.03 -01:19:01.3 -- a known variable star
06:41:46.37 -00:57:08.2 -- a known variable star
06:41:52.25 -05:30:57.4 -- not a known variable star
06:42:21.50 -05:13:54.2 -- not a known variable star
06:42:30.96 -06:04:21.5 -- a known variable star
06:42:33.16 -03:28:07.1 -- not a known variable star
06:42:36.24 +00:14:26.2 -- a known variable star
06:42:59.47 +00:50:06.0 -- not a known variable star
06:43:09.64 -02:13:05.6 -- not a known variable star
06:43:24.65 -00:26:07.7 -- not a known variable star
06:43:36.92 -04:25:01.8 -- a known variable star
06:43:47.08 +01:14:20.3 -- not a known variable star
06:43:55.46 -05:04:01.2 -- not a known variable star
06:43:56.53 -05:38:37.3 -- a known variable star
06:44:12.33 -00:00:20.9 -- not a known variable star
06:44:24.58 +01:58:58.7 -- not a known variable star
06:44:25.40 +01:06:41.5 -- not a known variable star
06:44:34.05 -01:35:29.2 -- a known variable star
06:44:38.28 -02:01:19.3 -- not a known variable star
06:44:50.61 +01:05:43.9 -- not a known variable star
06:44:57.65 -02:51:41.3 -- not a known variable star
06:44:58.53 +00:57:06.9 -- not a known variable star
06:45:06.88 -01:17:20.7 -- a known variable star
06:45:12.35 -00:01:51.7 -- not a known variable star
06:45:13.11 -00:39:27.0 -- not a known variable star
06:45:17.59 +00:43:39.8 -- not a known variable star
06:45:26.98 -05:18:36.6 -- not a known variable star
06:46:10.30 -03:13:58.6 -- a known variable star
06:46:13.87 +00:50:43.1 -- not a known variable star
06:46:32.58 -01:51:13.2 -- not a known variable star
06:46:46.43 -05:31:23.3 -- a known variable star
06:47:04.30 +01:23:25.1 -- not a known variable star
06:47:10.33 -05:37:12.4 -- not a known variable star
06:47:14.98 -05:48:24.9 -- not a known variable star
06:47:27.83 -01:05:51.7 -- a known variable star
06:47:32.90 +00:59:47.6 -- not a known variable star
06:48:34.64 -03:13:29.6 -- not a known variable star
06:48:43.87 -05:54:26.4 -- not a known variable star
06:48:50.55 -00:08:31.6 -- not a known variable star
06:48:53.17 +01:49:30.1 -- a known variable star
06:49:07.29 -01:40:16.8 -- not a known variable star
06:49:16.80 -00:21:50.7 -- not a known variable star
06:49:24.55 -00:56:17.3 -- not a known variable star
06:49:52.37 -02:39:52.7 -- not a known variable star
06:49:56.03 -02:17:02.2 -- not a known variable star
06:49:56.14 -02:40:55.2 -- not a known variable star
06:50:00.15 -05:55:19.0 -- not a known variable star
06:50:01.35 +01:08:24.2 -- not a known variable star
06:50:14.48 -00:47:12.5 -- not a known variable star
06:50:47.02 -05:49:03.5 -- a known variable star
06:50:57.40 -01:59:58.3 -- not a known variable star
06:51:05.03 -01:41:33.8 -- a known variable star
06:51:09.62 +00:53:03.1 -- not a known variable star
06:51:10.19 -02:40:57.4 -- not a known variable star
06:51:11.46 -02:22:09.8 -- not a known variable star
06:51:12.94 -00:35:21.7 -- a known variable star
06:51:17.94 -01:57:55.9 -- not a known variable star
06:51:23.95 +00:52:43.8 -- not a known variable star
06:51:34.31 -01:39:23.4 -- not a known variable star
06:51:35.01 -02:45:18.3 -- a known variable star
06:51:36.63 -02:04:10.2 -- a known variable star
06:51:43.41 -01:38:55.8 -- not a known variable star
06:51:52.90 -04:24:14.9 -- not a known variable star
06:51:59.94 +00:27:10.5 -- not a known variable star
06:52:01.72 -00:36:53.6 -- not a known variable star
06:52:50.97 -02:20:52.3 -- not a known variable star
06:52:55.15 -02:23:02.7 -- not a known variable star
06:53:04.48 -05:33:23.6 -- not a known variable star
06:53:05.79 -05:33:50.2 -- a known variable star
06:53:09.49 -01:41:54.9 -- not a known variable star
06:53:22.58 -03:34:22.9 -- not a known variable star
06:53:36.72 -02:31:47.7 -- a known variable star
06:53:41.39 -00:33:48.9 -- a known variable star
06:53:42.69 -03:34:07.5 -- a known variable star
06:53:43.52 -01:58:43.0 -- not a known variable star
06:53:48.85 -03:17:34.4 -- not a known variable star
06:53:51.71 -01:17:01.5 -- not a known variable star
06:54:03.07 -00:10:55.1 -- not a known variable star
06:54:06.80 -01:31:49.3 -- not a known variable star
06:54:17.81 -04:54:48.1 -- not a known variable star
06:54:22.80 -02:36:36.2 -- not a known variable star
06:54:23.36 -01:37:01.2 -- not a known variable star
06:54:40.57 -01:56:11.2 -- a known variable star
06:54:41.09 -02:07:02.0 -- a known variable star
06:54:48.38 +00:23:18.5 -- a known variable star
06:54:53.44 -01:04:23.5 -- a known variable star
06:54:59.11 -05:04:37.5 -- not a known variable star
06:55:07.46 -02:37:23.3 -- a known variable star
06:55:26.35 -02:12:44.7 -- not a known variable star
06:55:37.71 -05:35:29.8 -- a known variable star
06:55:50.64 -02:12:28.8 -- not a known variable star
06:56:04.48 -01:29:58.8 -- not a known variable star
06:56:22.04 -00:53:11.9 -- a known variable star
06:56:26.14 -02:53:13.1 -- not a known variable star
06:56:27.65 -01:27:43.3 -- not a known variable star
06:56:39.28 -02:13:31.3 -- not a known variable star
06:56:48.80 +02:10:37.6 -- not a known variable star
06:57:07.02 -00:31:51.4 -- a known variable star
06:57:12.43 -03:57:45.8 -- not a known variable star
06:57:16.55 -02:44:41.9 -- not a known variable star
06:57:24.11 -02:57:03.7 -- not a known variable star
06:57:27.82 -05:05:44.2 -- not a known variable star
06:57:35.71 +01:13:53.0 -- a known variable star
06:57:39.38 -03:34:43.4 -- not a known variable star
06:57:43.47 -02:07:57.6 -- a known variable star
06:57:55.61 -01:46:59.6 -- not a known variable star
06:58:00.35 -00:22:01.1 -- not a known variable star
06:58:00.70 -02:48:59.5 -- not a known variable star
06:58:09.42 -01:16:02.1 -- not a known variable star
06:58:20.38 -00:32:37.9 -- not a known variable star
06:58:34.68 -01:38:22.5 -- not a known variable star
06:58:35.47 -04:20:28.6 -- not a known variable star
06:58:39.26 -01:55:23.5 -- not a known variable star
06:58:43.29 -01:49:10.7 -- not a known variable star
06:58:50.15 -04:41:11.0 -- not a known variable star
06:58:57.09 -03:00:41.1 -- not a known variable star
06:59:01.00 -02:36:03.2 -- not a known variable star
06:59:04.01 -02:15:14.6 -- not a known variable star
06:59:30.37 +00:22:08.2 -- not a known variable star
07:00:00.11 -05:53:48.8 -- not a known variable star
07:00:09.69 -00:53:34.6 -- not a known variable star
07:01:12.29 -01:23:36.4 -- not a known variable star
07:01:14.75 -02:44:16.9 -- not a known variable star
07:01:15.25 -06:13:20.0 -- not a known variable star
07:01:33.73 -00:32:33.4 -- not a known variable star
07:01:43.84 -01:10:42.5 -- not a known variable star
07:01:56.11 +01:13:07.8 -- not a known variable star
07:02:05.77 -02:46:38.1 -- not a known variable star
07:02:12.49 -04:22:05.5 -- not a known variable star
07:02:21.42 -04:03:31.4 -- a known variable star
07:02:23.95 -01:34:38.3 -- not a known variable star
07:02:35.21 -06:06:06.7 -- not a known variable star
07:02:38.29 -04:51:08.1 -- not a known variable star
07:02:47.23 -03:51:37.0 -- not a known variable star
07:02:49.12 -05:28:13.9 -- not a known variable star
07:02:57.90 -00:25:26.1 -- not a known variable star
07:03:04.46 -01:18:38.1 -- not a known variable star
07:03:24.64 -05:00:15.5 -- a known variable star
07:03:25.13 -05:00:40.5 -- a known variable star
07:03:29.11 -01:38:50.4 -- a known variable star
07:03:34.51 -06:11:12.7 -- a known variable star
07:03:36.13 -03:22:58.9 -- not a known variable star
07:03:39.75 -04:38:24.0 -- not a known variable star
07:03:41.01 -02:10:57.3 -- a known variable star
07:03:41.07 -04:17:23.5 -- a known variable star
07:03:52.66 -06:00:23.9 -- not a known variable star
07:03:54.03 -00:56:59.2 -- not a known variable star
07:03:59.42 -05:30:49.0 -- a known variable star
07:04:05.58 +00:58:05.8 -- not a known variable star
07:04:16.84 -03:01:38.5 -- not a known variable star
07:04:42.38 -04:08:44.8 -- not a known variable star
07:04:56.01 -05:21:46.4 -- a known variable star
07:04:59.46 -05:12:08.6 -- not a known variable star
07:05:05.71 -03:34:37.0 -- not a known variable star
07:05:09.83 -06:04:37.2 -- a known variable star
07:05:25.41 -03:18:31.6 -- not a known variable star
07:05:50.92 -02:05:13.3 -- not a known variable star
07:06:13.29 -03:12:30.5 -- a known variable star
07:06:17.15 +02:00:15.1 -- not a known variable star
07:06:31.66 +01:08:37.7 -- a known variable star
07:06:42.33 -03:09:11.6 -- not a known variable star
07:06:46.66 -01:31:18.2 -- not a known variable star
07:06:47.91 -03:23:13.7 -- not a known variable star
07:06:50.26 +00:50:33.6 -- not a known variable star
07:06:51.81 -05:24:28.3 -- a known variable star
07:06:56.34 +00:23:24.0 -- not a known variable star
07:07:02.43 -01:57:17.0 -- a known variable star
07:07:08.46 -02:45:58.5 -- not a known variable star
07:07:42.94 -02:06:39.6 -- a known variable star
07:07:43.10 -02:39:44.4 -- not a known variable star
07:07:45.99 -03:10:12.5 -- not a known variable star
07:07:51.47 -05:46:59.9 -- a known variable star
07:08:17.19 -04:56:00.7 -- a known variable star
07:08:32.37 -04:39:28.8 -- a known variable star
07:08:43.28 -05:05:29.4 -- a known variable star
07:08:48.79 -03:42:58.7 -- not a known variable star
07:08:59.14 -00:34:33.0 -- a known variable star
07:09:03.27 -02:29:04.9 -- not a known variable star
07:09:08.41 -01:41:26.7 -- a known variable star
07:09:10.35 -01:30:23.0 -- a known variable star
07:09:14.02 -03:42:55.6 -- not a known variable star
07:09:26.58 -02:33:16.7 -- not a known variable star
07:09:27.13 -00:57:18.6 -- not a known variable star
07:09:51.92 -05:21:54.6 -- a known variable star
Found 143 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
199 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 199 (excluding asteroids and hot pixels, 143 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)2461149.61286255 -observatory V36
00:24:11.78 -00:14:59.3 Mercury (-0.1mag)
03:23:57.39 +18:59:10.5 Venus (-3.9mag)
00:26:40.48 +01:50:06.6 Mars (1.2mag)
07:14:05.80 +22:43:47.8 Jupiter (-2.1mag)
00:30:33.64 +00:57:33.5 Saturn (0.9mag)
03:48:21.65 +19:49:35.9 Uranus (5.8mag)
00:11:14.60 -00:12:50.2 Neptune (7.8mag)
20:33:52.85 -22:52:46.6 Pluto (14.5mag)
03:05:44.10 +22:14:04.8 Moon (-8.6mag)
-rw-r--r-- 1 apache apache 362 Apr 19 06:50 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461149.61286255:
07:13:58.46 +22:44:02.5 Io (5.8mag)
07:13:59.64 +22:44:03.5 Europa (5.9mag)
07:13:46.43 +22:44:28.9 Ganymede (5.4mag)
07:14:22.02 +22:43:05.5 Callisto (6.6mag)
07:17:17.53 +22:30:00.9 Himalia (15.4mag)
07:14:06.84 +22:43:47.6 Thebe (16.2mag)
07:17:32.74 +23:00:20.6 Elara (17.3mag)
07:13:11.38 +23:22:10.4 Pasiphae (17.4mag)
07:22:21.23 +22:42:06.6 Carme (18.5mag)
00:30:24.79 +00:57:55.6 Titan (8.8mag)
00:30:33.08 +00:57:49.6 Rhea (10.1mag)
00:30:08.96 +00:57:12.9 Iapetus (11.5mag)
00:30:29.87 +00:58:01.6 Hyperion (14.8mag)
00:32:08.01 +01:06:01.2 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 19 06:50 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461149.61286255:
15:51:31.39 -18:19:41.2 JWST
16:03:37.29 +50:15:00.4 Chandra
16:56:18.31 -51:26:35.2 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 19 06:50 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461149.61286255 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:53:09.79 -28:57:55.9 13.9mag P/2010 H2 (Vales)
05:09:00.88 -69:31:03.3 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:33:08.80 +31:27:33.3 17.2mag C/2017 K2 (PANSTARRS)
17:30:04.54 +10:54:47.5 17.6mag C/2021 G2 (ATLAS)
23:11:00.85 +29:21:19.1 17.1mag C/2022 E2 (ATLAS)
04:32:53.08 +26:07:17.7 16.0mag C/2022 N2 (PANSTARRS)
09:04:09.44 +32:01:47.0 16.2mag C/2022 QE78 (ATLAS)
08:31:36.24 +00:10:13.9 17.4mag C/2022 R6 (PANSTARRS)
18:52:56.00 +18:47:26.7 17.6mag C/2023 A3 (Tsuchinshan-ATLAS)
15:39:37.67 -11:28:32.6 17.5mag P/2023 B1 (PANSTARRS)
09:06:16.70 -11:23:32.1 17.7mag C/2023 F3 (ATLAS)
21:57:13.24 +63:05:35.5 17.5mag C/2023 H5 (Lemmon)
19:16:20.18 -03:47:22.4 14.1mag C/2023 R1 (PANSTARRS)
21:24:30.81 +86:20:50.4 17.8mag C/2023 X2 (Lemmon)
06:19:29.39 +63:30:11.5 17.2mag C/2024 A1 (ATLAS)
05:19:49.92 +19:17:34.9 11.3mag C/2024 E1 (Wierzchos)
16:17:13.06 +06:53:54.7 17.4mag C/2024 G6 (ATLAS)
20:21:36.66 +16:07:43.8 14.6mag C/2024 J3 (ATLAS)
03:29:11.27 -21:55:04.8 16.3mag C/2024 T5 (ATLAS)
05:19:23.26 +44:31:54.6 17.7mag C/2025 J1 (Borisov)
13:26:01.38 +47:19:39.0 15.3mag C/2025 L1 (ATLAS)
03:30:16.43 -26:42:28.0 17.9mag C/2025 Q3 (ATLAS)
00:17:30.50 +17:02:53.4 8.1mag C/2025 R3 (PANSTARRS)
12:52:46.99 +03:11:51.2 17.4mag C/2025 Y1 (ATLAS)
03:51:03.98 +02:20:11.8 14.2mag C/2026 A1 (MAPS)
00:08:16.92 +37:46:20.4 14.7mag C/2026 B2 (Sun-Gao)
18:48:59.10 -09:33:00.6 11.6mag 10P/Tempel
14:56:03.77 +02:52:09.9 14.3mag 24P/Schaumasse
11:02:01.25 -01:25:45.7 15.7mag 29P/Schwassmann-Wachmann
10:37:33.57 -03:51:44.8 17.0mag 43P/Wolf-Harrington
01:53:29.97 +18:00:54.1 17.3mag 47P/Ashbrook-Jackson
07:16:35.42 +36:20:16.7 17.0mag 63P/Wild
23:32:59.49 -11:04:51.9 15.7mag 65P/Gunn
04:11:39.24 +22:18:13.2 15.9mag 76P/West-Kohoutek-Ikemura
01:12:29.04 +08:50:13.9 14.3mag 78P/Gehrels
23:12:19.60 -08:28:11.9 14.7mag 88P/Howell
02:19:16.96 +21:27:33.4 15.1mag 93P/Lovas
05:00:45.14 +32:26:52.6 16.2mag 123P/West-Hartley
08:32:09.53 +36:55:37.2 16.2mag 124P/Mrkos
02:38:02.88 +14:42:50.5 16.4mag 128P/Shoemaker-Holt
02:53:39.51 +14:51:58.8 17.5mag 131P/Mueller
01:42:39.66 +14:16:22.4 10.5mag 141P/Machholz
01:51:06.83 +06:02:06.5 10.5mag 141P-A/Machholz
00:35:00.77 +01:50:59.7 12.4mag 141P-D/Machholz
02:21:38.47 +07:47:27.7 17.9mag 141P-I/Machholz
01:11:05.05 +00:02:39.3 15.0mag 162P/SidingSpring
14:45:55.75 +00:14:03.1 17.7mag 210P/Christensen
21:47:38.83 -10:42:08.5 17.7mag 218P/LINEAR
17:17:08.93 -13:33:18.5 16.1mag 235P/LINEAR
05:41:15.09 +34:55:15.9 16.8mag 240P/NEAT
07:40:05.56 -04:50:19.3 17.8mag 242P/Spahr
22:24:41.65 -20:08:02.7 17.8mag 260P/McNaught
02:04:35.71 +21:14:23.2 18.0mag 295P/LINEAR
15:41:22.24 +07:11:22.0 17.5mag 391P/Kowalski
07:35:27.33 +21:22:20.5 17.7mag 450P/LONEOS
05:40:27.46 +44:51:03.6 17.5mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.8K Apr 19 06:50 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
14:49:14.13 -27:29:20.60 ASASSN-26cu 2026-04-16.06 14.03
17:21:59.44 -38:54:04.60 ASASSN-26ct 2026-04-14.4 15.15
15:25:54.99 +07:49:24.50 SN2026huo 2026-04-12.14 16.96
14:49:14.13 -27:29:20.60 2026-04-16.06 14.03
12:23:20.40 +04:53:39.10 AT2026ixd 2026-04-12.14 17.65
17:46:09.76 -61:19:50.40 SN2026icy 2026-04-12.2 17.03
09:25:46.42 +02:13:46.30 SN2026gud 2026-04-11.98 16.49
16:52:15.46 -60:27:45.90 ASASSN-26cs 2026-04-12.4 15.5
04:20:55.37 -51:15:31.10 ASASSN-26cr 2026-04-12.01 15.37
22:25:39.35 +36:45:06.90 AT2026ihl 2026-04-10.48 14.21
19:40:44.94 +00:41:03.80 AT2026imw 2026-04-10.32 16.06
19:52:04.70 +05:53:33.50 ASASSN-26cq 2026-04-9.31 14.98
16:08:18.39 -64:11:08.80 ASASSN-26cp 2026-04-9.29 13.32
09:22:22.90 -61:02:43.70 SN2026idh 2026-04-7.97 16.34
05:06:54.12 -19:42:26.40 AT2026imr 2026-04-8 17.49
07:14:55.34 -36:03:21.40 AT2026hei 2026-04-8.12 16.7
21:35:33.14 -19:01:34.80 AT2026ihm 2026-04-8.36 16.7
04:28:24.08 -32:25:35.30 AT2026imo 2026-04-8.02 16.81
05:10:35.79 -39:38:40.80 SN 2026hnn 2026-04-7.04 17.07
09:54:32.04 -01:17:25.80 ASASSN-26cn 2026-04-7.01 15.58
07:46:24.43 -77:29:36.30 ASASSN-26co 2026-04-7.15 15.11
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.81 -27:51:50.40 SN2026gvk 2026-03-30 15.28
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.79 -63:44:05.60 ASASSN-26ch 2026-03-28.12 13.14
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.87 -53:16:33.70 ASASSN-26cc 2026-03-20.08 3.93
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.90 -45:55:38.40 ASASSN-26bt 2026-03-19.05 16.24
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.67 -47:26:43.70 ASASSN-26bn 2026-03-10.12 15.2
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.48 -37:49:32.80 ASASSN-26bk 2026-03-2.3 13.11
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.37 +19:58:46.70 ASASSN-26be 2026-02-25.58 14.8
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
-rw-r--r-- 1 apache apache 5.8K Apr 19 06:50 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 19 06:50 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
17:37:45.700 +39:48:28.26 AT 2026jjh 2026-04-07.87 20.39
16:35:21.390 +30:27:47.12 AT 2026jjg 2026-04-07.79 20.91
17:02:03.120 +41:30:38.89 AT 2026jjf 2026-04-03.89 21.38
17:08:30.580 +41:56:13.61 AT 2026jje 2026-04-03.89 21.47
16:48:25.780 +33:00:44.35 AT 2026jjd 2026-04-03.85 21.29
16:46:02.450 +30:55:42.15 AT 2026jjc 2026-04-03.80 19.57
16:51:04.120 +44:26:50.06 AT 2026jjb 2026-03-30.84 21.02
12:10:02.030 +43:26:37.06 AT 2026jja 2026-03-28.87 21.46
17:56:59.910 +48:20:04.31 AT 2026jiz 2026-03-27.87 20.99
15:23:12.550 +15:30:01.81 AT 2026jiy 2026-03-27.82 21.09
12:45:41.400 +53:52:15.13 AT 2026jix 2026-03-24.70 20.56
12:05:28.040 +47:18:05.03 AT 2026jiw 2026-03-24.69 20.17
12:49:49.680 +44:27:28.62 AT 2026jiv 2026-03-24.69 21.87
12:17:57.600 +45:03:04.77 AT 2026jiu 2026-03-24.69 20.4
11:39:16.940 +45:15:03.67 AT 2026jit 2026-03-24.66 21.06
14:17:33.100 +43:22:03.41 AT 2026jis 2026-03-22.80 20.74
14:45:33.130 +38:26:13.04 AT 2026jir 2026-03-22.80 21.14
14:42:55.800 +38:18:34.13 AT 2026jiq 2026-03-22.80 21.14
12:43:36.900 +28:13:26.06 AT 2026jip 2026-03-20.69 21.81
13:50:42.590 +38:45:33.09 AT 2026jio 2026-03-29.93 20.87
-rw-r--r-- 1 apache apache 30K Apr 19 06:50 tns_transients_list.txt
