This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 19.4427* 23 45 02.69 +43 55 27.1 10.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
EY And,2461149.9427,10.19,0.05,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
EY And 20260419.4427 10.19CV 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!
TCP 2026 04 19.4427* 23 50 51.99 +43 04 44.6 10.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
EZ And,2461149.9427,10.94,0.05,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
EZ And 20260419.4427 10.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 19.4427* 23 54 35.24 +43 11 17.5 11.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2354350+431115,2461149.9427,11.38,0.05,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
NSVS J2354350+431115 20260419.4427 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 19.4427* 23 49 13.42 +46 43 10.6 12.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.9427,12.46,0.05,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
target 20260419.4427 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 19.4427* 23 44 33.48 +43 14 28.6 11.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.9427,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.4427 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 19.4427* 00 11 06.94 +46 26 23.7 11.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.9427,11.85,0.05,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
target 20260419.4427 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!
TCP 2026 04 19.4427* 00 05 25.55 +44 17 04.4 11.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.9427,11.70,0.05,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 20260419.4427 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 19.4427* 23 39 29.81 +46 54 14.1 12.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.9427,12.16,0.05,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
target 20260419.4427 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!
TCP 2026 04 19.4427* 23 44 05.99 +49 20 23.0 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1940476983231943808,2461149.9427,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1940476983231943808 20260419.4427 12.19CV 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!
TCP 2026 04 19.4427* 00 20 21.28 +47 00 00.1 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 392085988201719296,2461149.9427,11.34,0.05,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 392085988201719296 20260419.4427 11.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 19.4427* 23 44 27.11 +49 42 05.4 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J356.1125+49.6989,2461149.9427,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J356.1125+49.6989 20260419.4427 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 19.4427* 23 48 52.06 +42 06 27.2 11.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1922492890007272448,2461149.9427,11.55,0.05,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 1922492890007272448 20260419.4427 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 19.4427* 23 37 29.63 +49 59 55.6 11.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1943698346142347136,2461149.9427,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1943698346142347136 20260419.4427 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 19.4427* 00 14 42.13 +46 51 21.8 10.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 392207548658221312,2461149.9427,10.93,0.05,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 392207548658221312 20260419.4427 10.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 19.4427* 23 36 37.63 +45 39 10.0 11.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1938876987652904960,2461149.9427,11.12,0.05,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 1938876987652904960 20260419.4427 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 19.4427* 23 48 36.96 +46 14 52.8 10.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J357.1393+46.2405,2461149.9427,9.96,0.05,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
ATO J357.1393+46.2405 20260419.4427 9.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 19.4427* 23 41 22.84 +46 52 23.1 10.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1939240926002369536,2461149.9427,10.07,0.05,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 1939240926002369536 20260419.4427 10.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 19.4427* 23 51 59.05 +49 01 25.1 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx2957648,2461149.9427,10.60,0.05,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
DocumentRef: VOTx2957648 20260419.4427 10.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 19.4427* 23 40 11.10 +45 02 54.6 10.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1926756143267842048,2461149.9427,10.75,0.05,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 1926756143267842048 20260419.4427 10.75CV 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!
TCP 2026 04 19.4427* 23 48 29.85 +46 16 21.1 10.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1927284797904773120,2461149.9427,10.86,0.05,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 1927284797904773120 20260419.4427 10.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 19.4427* 23 42 09.74 +44 44 15.5 10.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1926630524064281088,2461149.9427,10.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1926630524064281088 20260419.4427 10.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 19.4427* 00 10 16.93 +49 00 00.6 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 393561876404915840,2461149.9427,11.03,0.05,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 393561876404915840 20260419.4427 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 19.4427* 23 39 25.83 +45 44 12.7 11.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.9427,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.4427 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 19.4427* 23 48 13.28 +47 05 59.6 11.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.9427,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.4427 11.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 19.4427* 00 02 09.78 +42 08 05.9 11.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.9427,11.06,0.05,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
target 20260419.4427 11.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 19.4427* 23 40 11.61 +48 47 39.7 11.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1940343186409018112,2461149.9427,11.54,0.05,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
Gaia DR3 1940343186409018112 20260419.4427 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 19.4427* 23 43 18.01 +43 20 59.1 11.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.9427,11.49,0.05,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
target 20260419.4427 11.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 19.4427* 23 43 32.16 +47 19 20.5 11.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.9427,11.65,0.05,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 20260419.4427 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 19.4427* 23 36 51.97 +43 17 18.3 11.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx2988042,2461149.9427,11.74,0.05,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
DocumentRef: VOTx2988042 20260419.4427 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 19.4427* 23 43 26.90 +47 19 48.7 11.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.9427,11.85,0.05,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
target 20260419.4427 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!
TCP 2026 04 19.4427* 00 02 11.49 +50 19 51.5 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx3071897,2461149.9427,11.70,0.05,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
DocumentRef: VOTx3071897 20260419.4427 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 19.4427* 23 43 18.55 +43 20 20.7 11.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.9427,11.69,0.05,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
target 20260419.4427 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!
TCP 2026 04 19.4427* 23 48 38.73 +43 37 22.6 11.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1925857739185928320,2461149.9427,11.66,0.05,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 1925857739185928320 20260419.4427 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 19.4427* 23 40 08.97 +49 47 07.0 12.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1943726658567506304,2461149.9427,12.03,0.05,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 1943726658567506304 20260419.4427 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 19.4427* 00 09 09.48 +49 47 10.0 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx3064923,2461149.9427,11.67,0.05,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
DocumentRef: VOTx3064923 20260419.4427 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!
TCP 2026 04 19.4427* 00 17 36.20 +50 17 52.3 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.9427,11.57,0.05,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
target 20260419.4427 11.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 19.4427* 23 38 10.23 +46 10 53.7 12.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1939093763243856896,2461149.9427,12.07,0.05,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 1939093763243856896 20260419.4427 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 19.4427* 00 01 22.66 +46 44 46.7 11.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.9427,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260419.4427 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 19.4427* 23 55 38.15 +48 37 54.5 11.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J358.9167+48.6202,2461149.9427,11.88,0.05,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 J358.9167+48.6202 20260419.4427 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 19.4427* 23 50 22.73 +50 15 37.0 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.9427,12.09,0.05,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
target 20260419.4427 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 19.4427* 23 38 10.45 +46 47 20.7 12.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1939180865179285248,2461149.9427,12.07,0.05,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 1939180865179285248 20260419.4427 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 19.4427* 23 35 06.16 +47 31 11.1 12.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx3120196,2461149.9427,12.14,0.05,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
DocumentRef: VOTx3120196 20260419.4427 12.14CV 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!
TCP 2026 04 19.4427* 23 39 17.32 +44 07 56.8 12.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx3123106,2461149.9427,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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: VOTx3123106 20260419.4427 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 19.4427* 00 03 56.36 +49 40 51.0 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx3124092,2461149.9427,12.05,0.05,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
DocumentRef: VOTx3124092 20260419.4427 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 19.4427* 23 45 02.95 +44 47 30.5 12.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.9427,12.10,0.05,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
target 20260419.4427 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!
TCP 2026 04 19.4427* 23 54 02.16 +44 33 34.6 12.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.9427,12.12,0.05,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
target 20260419.4427 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!
TCP 2026 04 19.4427* 23 54 40.83 +44 53 44.4 12.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.9427,12.00,0.05,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
target 20260419.4427 12.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 19.4427* 00 17 32.61 +45 44 45.0 11.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx3086029,2461149.9427,11.80,0.05,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
DocumentRef: VOTx3086029 20260419.4427 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 19.4427* 23 35 22.96 +45 57 49.4 12.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DocumentRef: VOTx3186325,2461149.9427,12.29,0.05,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
DocumentRef: VOTx3186325 20260419.4427 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 19.4427* 23 50 36.77 +47 03 37.0 12.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J357.6483+47.0604,2461149.9427,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J357.6483+47.0604 20260419.4427 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 19.4427* 23 50 20.38 +46 56 39.5 12.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J357.5823+46.9470,2461149.9427,12.27,0.05,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
ATO J357.5823+46.9470 20260419.4427 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 19.4427* 23 50 34.35 +43 04 29.6 12.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J235034.15+430430.1,2461149.9427,11.96,0.05,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
ASASSN-V J235034.15+430430.1 20260419.4427 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 19.4427* 00 25 37.48 +47 12 42.8 9.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J002537.73+471244.7,2461149.9427,9.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J002537.73+471244.7 20260419.4427 9.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 19.4427* 23 42 09.19 +46 24 30.9 10.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0697 And,2461149.9427,10.07,0.05,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
V0697 And 20260419.4427 10.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 19.4427* 23 34 07.85 +46 20 01.1 10.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0339 And,2461149.9427,10.69,0.05,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
V0339 And 20260419.4427 10.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 19.4427* 23 39 52.00 +47 45 01.8 11.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
EX And,2461149.9427,10.97,0.05,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
EX And 20260419.4427 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461036.57699117 27.12.2025 01:50:42.037 /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
First image: 2461036.57699117 27.12.2025 01:50:42.037 /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
Last image: 2461149.94299415 19.04.2026 10:37:44.695 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 12
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.88
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: 14 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): 19081
Objects passed selection criteria: 19000
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 13539.5
Average stars matched: 12269.2 (90.6182 %)
Memory usage VmPeak: 121816 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 05:40:27 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: 2461036.57699117 27.12.2025 01:50:42.037 /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
First image: 2461036.57699117 27.12.2025 01:50:42.037 /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
Last image: 2461149.94299415 19.04.2026 10:37:44.695 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 121
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.48
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: 58 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): 118495
Objects passed selection criteria: 118147
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 85362.2
Average stars matched: 77305.8 (90.562 %)
Memory usage VmPeak: 1941724 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 05:44:32 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/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits
SExtractor catalog cache: saved And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits.cat to cache
SExtractor catalog cache: saved And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.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/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.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: 2461149.94236278
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_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits exists and is non-empty
Saving wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits to local_wcs_cache/
'wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits' -> 'local_wcs_cache/wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits'
wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits exists and is non-empty
Saving wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits to local_wcs_cache/
'wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits' -> 'local_wcs_cache/wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits'
wcs_fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits exists and is non-empty
Saving wcs_fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits to local_wcs_cache/
'wcs_fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits' -> 'local_wcs_cache/wcs_fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits'
wcs_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits exists and is non-empty
Saving wcs_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits to local_wcs_cache/
'wcs_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits' -> 'local_wcs_cache/wcs_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits (1st reference image)
verification OK: wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
Image size: 924.9'x628.2' 15.4(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.80"/pix along the X axis and 5.90"/pix along the Y axis
Image center: 00:00:19.361 +45:58:07.34 J2000 4789.000 3195.000
###################################
The image scale is 5.80"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.7"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits (1st new image)
verification OK: wcs_fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits
Image size: 939.1'x624.2' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:00:01.553 +46:03:15.92 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:00:19.361 +45:58:07.34
Second-epoch image center 00:00:01.553 +46:03:15.92
Angular distance between the image centers 0.1000 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits (2nd new image)
verification OK: wcs_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits
Image size: 939.0'x624.2' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:59:59.033 +46:03:56.22 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:00:19.361 +45:58:07.34
Second-epoch image center 23:59:59.033 +46:03:56.22
Angular distance between the image centers 0.1134 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 00:00:01.553 +46:03:15.92
Second-epoch second image center 23:59:59.033 +46:03:56.22
Angular distance between the image centers 0.01336 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/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits &> /tmp/tmp.0mHhjp8jvG
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits &> /tmp/tmp.bgP1BQEOiA
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits &> /tmp/tmp.zedA8p6mYx
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits &> /tmp/tmp.JWhK6HPkQI
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits
Calibrating the magnitude scale
Found non-empty wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.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_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits and wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.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_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits and wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits.cat
Found non-empty wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits and wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits.cat
The reference image (wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits) and catalog (wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits.cat) found
'wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits.cat' -> 'wcsmag.cat'
Read 21978 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0038 to 359.9998 deg, Dec +39.9518 to +51.2135 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 0.0038 to 359.9998 deg, Dec 39.9518 to 51.2135 deg
Loaded 169717 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): 58 out of 66 total matches.
Matched with Tycho-2 66 out of 21978 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.835338
a=0.000000 b=1.000000 c=22.835338
From vast_summary.log: estimated ref. image limiting mag.: -7.88
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.96
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.96
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 8 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.5 pix And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
2.5 pix And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
2.9 pix fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits
3.0 pix fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits
Limiting magnitude estimates:
15.0 mag. And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
15.0 mag. And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
14.1 mag. fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits
14.1 mag. fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 11.5 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.0mHhjp8jvG (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/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.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_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits 567.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits' -> 'wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
WCS_IMAGE_NAME=wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
WCS-calibrated image found: wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
Checking if the catalog wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits.cat corresponding to the image wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits alredy exist and is non-empty...
Catalog wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits.cat corresponding to the image wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
WCS catalog name: wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2256, passed=21978
Got 21978 stars (including 19693 good ones) from the SExtractor catalog wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits.cat
util/solve_plate_with_UCAC5 got 21978 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 924.9'
Seting catalog search parameters based on the expected field of view 924.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012846 (46.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010277 (37.0 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 348.4507 through 0 to 12.6948, gap 12.6948 to 348.4507
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 40.0 to 51.2)
Done reading UCAC5 zone files...
Matched 203 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 146 matched stars entering correct_measured_positions(), 68 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 10.79"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 141 matched stars entering correct_measured_positions(), 2320 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 11.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 348.4573 through 0 to 12.6998, gap 12.6998 to 348.4573
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 40.0 to 51.2)
Done reading UCAC5 zone files...
Matched 230 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 175 matched stars entering correct_measured_positions(), 2338 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 11.32"
Accuracy estimation diagnostic: 173 matched stars entering correct_measured_positions(), 3009 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.42"
Excluding outliers - 173 stars left (next iteration limit 155)
The image catalog is written to wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits -region wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.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.bgP1BQEOiA (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/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.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_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits 567.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits' -> 'wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
WCS_IMAGE_NAME=wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
WCS-calibrated image found: wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
Checking if the catalog wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits.cat corresponding to the image wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits alredy exist and is non-empty...
Catalog wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits.cat corresponding to the image wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
WCS catalog name: wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2250, passed=22050
Got 22050 stars (including 19777 good ones) from the SExtractor catalog wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits.cat
util/solve_plate_with_UCAC5 got 22050 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 924.9'
Seting catalog search parameters based on the expected field of view 924.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012846 (46.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010277 (37.0 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 348.4512 through 0 to 12.6947, gap 12.6947 to 348.4512
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 40.0 to 51.2)
Done reading UCAC5 zone files...
Matched 202 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 142 matched stars entering correct_measured_positions(), 69 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 11.99"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 135 matched stars entering correct_measured_positions(), 2248 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 12.05"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 348.4583 through 0 to 12.7006, gap 12.7006 to 348.4583
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 40.0 to 51.2)
Done reading UCAC5 zone files...
Matched 223 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 175 matched stars entering correct_measured_positions(), 2273 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 12.04"
Accuracy estimation diagnostic: 172 matched stars entering correct_measured_positions(), 3100 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 10.65"
Excluding outliers - 172 stars left (next iteration limit 148)
The image catalog is written to wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits -region wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.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.zedA8p6mYx (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_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.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_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits
WCS_IMAGE_NAME=wcs_fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits
WCS-calibrated image found: wcs_fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits
Checking if the catalog wcs_fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits.cat corresponding to the image wcs_fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits alredy exist and is non-empty...
Catalog wcs_fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits.cat corresponding to the image wcs_fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits
WCS catalog name: wcs_fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=914, passed=12420
Got 12420 stars (including 11499 good ones) from the SExtractor catalog wcs_fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits.cat
util/solve_plate_with_UCAC5 got 12420 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.1'
Seting catalog search parameters based on the expected field of view 939.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013043 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010434 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 347.5148 through 0 to 12.2291, gap 12.2291 to 347.5148
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.3 to 51.3)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 907 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.90"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 11955 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.91"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 347.5148 through 0 to 12.2299, gap 12.2299 to 347.5148
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.3 to 51.3)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 11954 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.92"
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 11954 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.98"
Excluding outliers - 935 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits -region wcs_fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.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.JWhK6HPkQI (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_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.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_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits
WCS_IMAGE_NAME=wcs_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits
WCS-calibrated image found: wcs_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits
Checking if the catalog wcs_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits.cat corresponding to the image wcs_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits alredy exist and is non-empty...
Catalog wcs_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits.cat corresponding to the image wcs_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits
WCS catalog name: wcs_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=908, passed=12487
Got 12487 stars (including 11574 good ones) from the SExtractor catalog wcs_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits.cat
util/solve_plate_with_UCAC5 got 12487 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.0'
Seting catalog search parameters based on the expected field of view 939.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013042 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010433 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 347.4705 through 0 to 12.1240, gap 12.1240 to 347.4705
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.3 to 51.3)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 908 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.93"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 12046 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.93"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 347.4702 through 0 to 12.1274, gap 12.1274 to 347.4702
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.3 to 51.3)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 12046 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.93"
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 12024 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.97"
Excluding outliers - 935 stars left (next iteration limit 1029)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits -region wcs_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.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_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits'
Saving fully-calibrated image wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits'
Saving fully-calibrated image wcs_fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/wcs_fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits'
Saving fully-calibrated image wcs_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/wcs_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits'
Preparing the HTML report for the field And-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out12192.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out18018.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31760.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32705.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 9s
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: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31760_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 31760_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31839_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
The candidate 31839_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745 did not pass the final checks
**** FOUND 00:12:06.63 +48:12:19.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32705_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 32705_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07730_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
The candidate 07730_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745 did not pass the final checks
**** FOUND 00:10:54.96 +48:15:31.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19449_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
The candidate 19449_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745 did not pass the final checks
**** FOUND 00:04:30.32 +42:07:14.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12192_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
The candidate 12192_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745 did not pass the final checks
**** FOUND 23:42:09.17 +46:24:31.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.38, MAG_FAINT_SEARCH_LIMIT=12.36)GAIADR2_OUTPUT=# 2.827 1939016213313882368 355.53784837941 +46.40941177209 10.3502 8.8876 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.827#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18018_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 18018_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15590_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
The candidate 15590_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745 did not pass the final checks
**** FOUND 00:22:05.08 +44:08:44.7 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 11s
Prepared the HTML report for the field And-01-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 ####
23:54:35.24 +43:11:17.5
23:45:02.69 +43:55:27.1
23:50:51.99 +43:04:44.6
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/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits
SExtractor catalog cache: saved And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits.cat to cache
SExtractor catalog cache: saved And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
Creating symlink local_wcs_cache/wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
Creating symlink local_wcs_cache/wcs_fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits
Creating symlink local_wcs_cache/wcs_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.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_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits exists and is non-empty
wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits exists and is non-empty
wcs_fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits exists and is non-empty
wcs_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits (1st reference image)
verification OK: wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
Image size: 924.9'x628.2' 15.4(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.80"/pix along the X axis and 5.90"/pix along the Y axis
Image center: 00:00:19.361 +45:58:07.34 J2000 4789.000 3195.000
###################################
The image scale is 5.80"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.7"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits (1st new image)
verification OK: wcs_fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits
Image size: 939.1'x624.2' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:00:01.553 +46:03:15.92 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:00:19.361 +45:58:07.34
Second-epoch image center 00:00:01.553 +46:03:15.92
Angular distance between the image centers 0.1000 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits (2nd new image)
verification OK: wcs_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits
Image size: 939.0'x624.2' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:59:59.033 +46:03:56.22 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:00:19.361 +45:58:07.34
Second-epoch image center 23:59:59.033 +46:03:56.22
Angular distance between the image centers 0.1134 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 00:00:01.553 +46:03:15.92
Second-epoch second image center 23:59:59.033 +46:03:56.22
Angular distance between the image centers 0.01336 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/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits &> /tmp/tmp.DPTQQRhEIL
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits &> /tmp/tmp.TCIjLQDkrz
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits &> /tmp/tmp.7GhKE7nm8J
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits &> /tmp/tmp.kluLlv5QCx
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits
Calibrating the magnitude scale
Found non-empty wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.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_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits and wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.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_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits and wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits.cat
Found non-empty wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits and wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits.cat
The reference image (wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits) and catalog (wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits.cat) found
'wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits.cat' -> 'wcsmag.cat'
Read 142009 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0001 to 359.9998 deg, Dec +39.9057 to +51.2155 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 0.0001 to 359.9998 deg, Dec 39.9057 to 51.2155 deg
Loaded 170564 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): 91 out of 117 total matches.
Matched with Tycho-2 117 out of 142009 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 21.227567
a=0.000000 b=1.000000 c=21.227567
From vast_summary.log: estimated ref. image limiting mag.: -7.48
Updating vast_summary.log: Estimated ref. image limiting mag.: 13.75
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 13.75
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 94 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
2.2 pix And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
2.9 pix fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits
2.9 pix fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits
Limiting magnitude estimates:
13.7 mag. And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
13.7 mag. And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
12.7 mag. fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits
12.7 mag. fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits
All-image limiting magnitude estimate: 12.7 (SNR ) 12.2 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.DPTQQRhEIL (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/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.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_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits 567.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits' -> 'wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
WCS_IMAGE_NAME=wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
WCS-calibrated image found: wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
Checking if the catalog wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits.cat corresponding to the image wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits alredy exist and is non-empty...
Catalog wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits.cat corresponding to the image wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
WCS catalog name: wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=47, blended=18012, passed=141962
Got 141962 stars (including 123722 good ones) from the SExtractor catalog wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits.cat
util/solve_plate_with_UCAC5 got 141962 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 924.9'
Seting catalog search parameters based on the expected field of view 924.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012846 (46.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010277 (37.0 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 348.4418 through 0 to 12.7147, gap 12.7147 to 348.4418
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.2)
Done reading UCAC5 zone files...
Matched 204 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 151 matched stars entering correct_measured_positions(), 79 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 10.98"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 145 matched stars entering correct_measured_positions(), 15623 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 12.14"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 348.4528 through 0 to 12.7273, gap 12.7273 to 348.4528
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.2)
Done reading UCAC5 zone files...
Matched 220 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 178 matched stars entering correct_measured_positions(), 15632 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 12.13"
Accuracy estimation diagnostic: 177 matched stars entering correct_measured_positions(), 18852 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 10.12"
Excluding outliers - 177 stars left (next iteration limit 159)
The image catalog is written to wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits -region wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.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.TCIjLQDkrz (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/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.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_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits 567.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits' -> 'wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
WCS_IMAGE_NAME=wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
WCS-calibrated image found: wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
Checking if the catalog wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits.cat corresponding to the image wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits alredy exist and is non-empty...
Catalog wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits.cat corresponding to the image wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
WCS catalog name: wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=51, blended=18105, passed=141752
Got 141752 stars (including 123429 good ones) from the SExtractor catalog wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits.cat
util/solve_plate_with_UCAC5 got 141752 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 924.9'
Seting catalog search parameters based on the expected field of view 924.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012846 (46.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010277 (37.0 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 348.4216 through 0 to 12.6947, gap 12.6947 to 348.4216
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.2)
Done reading UCAC5 zone files...
Matched 199 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 147 matched stars entering correct_measured_positions(), 78 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 11.76"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 141 matched stars entering correct_measured_positions(), 15342 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 11.76"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 348.4333 through 0 to 12.6945, gap 12.6945 to 348.4333
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.2)
Done reading UCAC5 zone files...
Matched 222 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 177 matched stars entering correct_measured_positions(), 15356 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 11.73"
Accuracy estimation diagnostic: 176 matched stars entering correct_measured_positions(), 20031 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 10.04"
Excluding outliers - 176 stars left (next iteration limit 155)
The image catalog is written to wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits -region wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.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.7GhKE7nm8J (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_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.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_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits
WCS_IMAGE_NAME=wcs_fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits
WCS-calibrated image found: wcs_fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits
Checking if the catalog wcs_fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits.cat corresponding to the image wcs_fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits alredy exist and is non-empty...
Catalog wcs_fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits.cat corresponding to the image wcs_fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits
WCS catalog name: wcs_fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=7003, passed=68471
Got 68471 stars (including 61379 good ones) from the SExtractor catalog wcs_fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits.cat
util/solve_plate_with_UCAC5 got 68471 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.1'
Seting catalog search parameters based on the expected field of view 939.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013043 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010434 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 347.4793 through 0 to 12.2290, gap 12.2290 to 347.4793
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.3 to 51.3)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 903 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.89"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 66167 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.88"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 347.4796 through 0 to 12.2307, gap 12.2307 to 347.4796
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.3 to 51.3)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 66169 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.88"
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 66085 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.97"
Excluding outliers - 934 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits -region wcs_fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.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.kluLlv5QCx (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_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.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_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits
WCS_IMAGE_NAME=wcs_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits
WCS-calibrated image found: wcs_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits
Checking if the catalog wcs_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits.cat corresponding to the image wcs_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits alredy exist and is non-empty...
Catalog wcs_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits.cat corresponding to the image wcs_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits
WCS catalog name: wcs_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=7092, passed=69371
Got 69371 stars (including 62211 good ones) from the SExtractor catalog wcs_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits.cat
util/solve_plate_with_UCAC5 got 69371 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.0'
Seting catalog search parameters based on the expected field of view 939.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013042 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010433 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 347.4706 through 0 to 12.1680, gap 12.1680 to 347.4706
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.3 to 51.3)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 904 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.90"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 66711 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.89"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 347.4703 through 0 to 12.1692, gap 12.1692 to 347.4703
Reading UCAC5 zone files...
Searching UCAC5 zones 651 to 708 (Dec 40.2 to 51.3)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 66707 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.89"
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 66706 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.98"
Excluding outliers - 934 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits -region wcs_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.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_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.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_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
Saving fully-calibrated image wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.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_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
Saving fully-calibrated image wcs_fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.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_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/wcs_fd_And-01-Q2b1x1_2026-04-19_05-36-50_20.00sec_-4.90C_LIGHT_0744.fits
Saving fully-calibrated image wcs_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.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_2026-04-19_CI_And-01-Q2b1x1_053820_TTUQ2b1x1_2586715_Aj20Z76o/wcs_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745.fits
Preparing the HTML report for the field And-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_local.txt__out116114.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161717.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161721.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161726.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161727.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161730.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161740.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161744.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161747.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161752.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161755.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161758.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161760.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161762.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out164468.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out166258.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out166870.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167623.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168002.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169313.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169570.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out170381.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out170716.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out170746.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out172420.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out172457.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out172841.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173513.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173524.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173595.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173632.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out174031.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out174036.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out174111.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175263.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175504.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175507.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175905.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175943.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176124.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176470.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177548.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177903.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out178187.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out178285.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out178318.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out179186.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out179595.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out179655.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57324.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57690.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out76104.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77205.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 494s
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: 52s
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Considering the candidate 161717_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 161717_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
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Considering the candidate 161721_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 161721_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
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Considering the candidate 161726_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 161726_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
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Considering the candidate 161727_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 161727_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
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Considering the candidate 161730_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 161730_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
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Considering the candidate 161740_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 161740_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
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Considering the candidate 161744_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 161744_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
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Considering the candidate 161747_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 161747_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
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Considering the candidate 161752_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 161752_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
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Considering the candidate 161755_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 161755_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
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Considering the candidate 161758_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 161758_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
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Considering the candidate 161760_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 161760_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
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Considering the candidate 161762_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 161762_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
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Considering the candidate 162705_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
The candidate 162705_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745 did not pass the final checks
**** FOUND 23:45:02.69 +43:55:27.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 162737_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
The candidate 162737_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745 did not pass the final checks
**** FOUND 00:12:06.57 +48:12:19.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 163586_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
The candidate 163586_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745 did not pass the final checks
**** FOUND 23:50:51.98 +43:04:45.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 164468_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 164468_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166258_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 166258_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
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Considering the candidate 166562_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
The candidate 166562_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745 did not pass the final checks
**** FOUND 23:38:07.53 +46:11:05.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 166742_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
The candidate 166742_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745 did not pass the final checks
**** FOUND 23:38:00.32 +46:13:35.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 166870_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 166870_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
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Considering the candidate 167623_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 167623_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
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Considering the candidate 168002_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 168002_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168107_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
The candidate 168107_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745 did not pass the final checks
**** FOUND 23:37:36.94 +44:27:13.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 168706_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
The candidate 168706_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745 did not pass the final checks
**** FOUND 00:05:31.47 +48:29:21.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 168847_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
The candidate 168847_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745 did not pass the final checks
**** FOUND 23:38:12.60 +43:17:59.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 168941_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
The candidate 168941_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745 did not pass the final checks
**** FOUND 23:50:38.03 +47:30:33.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 169313_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 169313_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 169570_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 169570_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
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Considering the candidate 170381_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 170381_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170431_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
The candidate 170431_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745 did not pass the final checks
**** FOUND 23:37:41.43 +44:25:25.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 170502_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
The candidate 170502_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745 did not pass the final checks
**** FOUND 00:12:00.22 +48:07:14.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 170716_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 170716_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170746_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 170746_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171157_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
The candidate 171157_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745 did not pass the final checks
**** FOUND 00:05:48.40 +45:47:25.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 171733_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
The candidate 171733_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745 did not pass the final checks
**** FOUND 00:03:20.95 +49:54:42.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 172273_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
The candidate 172273_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745 did not pass the final checks
**** FOUND 23:50:07.77 +47:35:51.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 172420_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 172420_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 172457_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 172457_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 172653_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
The candidate 172653_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745 did not pass the final checks
**** FOUND 23:37:34.05 +44:24:07.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 172841_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 172841_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173513_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 173513_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173524_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 173524_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173540_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
The candidate 173540_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745 did not pass the final checks
**** FOUND 00:04:16.86 +49:58:43.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173595_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 173595_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173632_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 173632_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173912_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
The candidate 173912_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745 did not pass the final checks
**** FOUND 23:44:32.02 +50:03:09.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174031_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 174031_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 174036_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 174036_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 174111_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 174111_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 174298_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
The candidate 174298_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745 did not pass the final checks
**** FOUND 00:09:56.62 +46:22:42.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174453_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
The candidate 174453_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745 did not pass the final checks
**** FOUND 23:54:40.46 +49:16:55.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 174523_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
The candidate 174523_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745 did not pass the final checks
**** FOUND 00:17:32.81 +50:15:57.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 175127_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
The candidate 175127_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745 did not pass the final checks
**** FOUND 00:18:30.56 +43:59:37.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 175263_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 175263_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 175283_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
The candidate 175283_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745 did not pass the final checks
**** FOUND 00:13:03.05 +49:56:52.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 175504_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 175504_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 175507_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 175507_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 175905_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 175905_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 175920_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
The candidate 175920_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745 did not pass the final checks
**** FOUND 00:10:11.77 +47:18:58.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 175943_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 175943_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 176124_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 176124_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 176470_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 176470_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 176743_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
The candidate 176743_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745 did not pass the final checks
**** FOUND 00:01:32.00 +47:56:36.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177150_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
The candidate 177150_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745 did not pass the final checks
**** FOUND 00:05:30.47 +46:40:47.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177548_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 177548_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177811_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
The candidate 177811_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745 did not pass the final checks
**** FOUND 00:06:30.11 +47:24:59.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177903_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 177903_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178187_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 178187_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178285_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 178285_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178288_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
The candidate 178288_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745 did not pass the final checks
**** FOUND 00:08:32.31 +46:07:24.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 178318_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 178318_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 179186_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 179186_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 179595_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 179595_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 179655_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 179655_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 180097_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
The candidate 180097_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745 did not pass the final checks
**** FOUND 00:05:35.41 +43:22:47.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 116114_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 116114_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46096_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
The candidate 46096_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745 did not pass the final checks
**** FOUND 00:10:54.90 +48:15:31.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 85909_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
The candidate 85909_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745 did not pass the final checks
**** FOUND 00:13:52.53 +45:26:32.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137188_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
The candidate 137188_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745 did not pass the final checks
**** FOUND 00:22:04.72 +44:08:42.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57690_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 57690_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52886_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
The candidate 52886_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745 did not pass the final checks
**** FOUND 00:19:50.32 +47:42:37.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 59955_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
The candidate 59955_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745 did not pass the final checks
**** FOUND 23:50:36.23 +47:31:25.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 108598_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
The candidate 108598_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745 did not pass the final checks
**** FOUND 00:17:10.64 +42:14:42.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 91789_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
The candidate 91789_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745 did not pass the final checks
**** FOUND 00:21:48.93 +44:52:17.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24383_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
The candidate 24383_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745 did not pass the final checks
**** FOUND 00:26:51.20 +49:10:15.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137934_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
The candidate 137934_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745 did not pass the final checks
**** FOUND 00:14:20.32 +44:20:30.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125310_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
The candidate 125310_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745 did not pass the final checks
**** FOUND 00:20:45.39 +43:21:19.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 76104_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 76104_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 77205_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 77205_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118010_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
The candidate 118010_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745 did not pass the final checks
**** FOUND 23:54:35.25 +43:11:17.7 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 117622_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
The candidate 117622_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745 did not pass the final checks
**** FOUND 00:04:30.32 +42:07:14.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57324_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
Preparing report for the candidate 57324_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70846_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745
The candidate 70846_fd_And-01-Q2b1x1_2026-04-19_05-37-44_20.00sec_-4.90C_LIGHT_0745 did not pass the final checks
**** FOUND 00:13:17.43 +46:24:54.6 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 14s
make_report_in_HTML.sh TOTAL: 560s
Prepared the HTML report for the field And-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
23:54:35.24 +43:11:17.5
23:45:02.69 +43:55:27.1
23:50:51.99 +43:04:44.6
23:50:34.35 +43:04:29.6
23:49:13.42 +46:43:10.6
23:44:33.48 +43:14:28.6
00:11:06.94 +46:26:23.7
00:05:25.55 +44:17:04.4
23:39:29.81 +46:54:14.1
23:44:05.99 +49:20:23.0
00:20:21.28 +47:00:00.1
23:44:27.11 +49:42:05.4
23:48:52.06 +42:06:27.2
23:37:29.63 +49:59:55.6
00:14:42.13 +46:51:21.8
23:36:37.63 +45:39:10.0
23:48:36.96 +46:14:52.8
23:41:22.84 +46:52:23.1
23:51:59.05 +49:01:25.1
23:40:11.10 +45:02:54.6
23:48:29.85 +46:16:21.1
23:42:09.74 +44:44:15.5
00:10:16.93 +49:00:00.6
23:39:25.83 +45:44:12.7
23:48:13.28 +47:05:59.6
00:02:09.78 +42:08:05.9
23:40:11.61 +48:47:39.7
23:43:18.01 +43:20:59.1
23:43:32.16 +47:19:20.5
23:36:51.97 +43:17:18.3
23:43:26.90 +47:19:48.7
00:02:11.49 +50:19:51.5
23:43:18.55 +43:20:20.7
23:48:38.73 +43:37:22.6
23:40:08.97 +49:47:07.0
00:09:09.48 +49:47:10.0
00:17:36.20 +50:17:52.3
23:38:10.23 +46:10:53.7
00:01:22.66 +46:44:46.7
23:55:38.15 +48:37:54.5
23:50:22.73 +50:15:37.0
23:38:10.45 +46:47:20.7
23:35:06.16 +47:31:11.1
23:39:17.32 +44:07:56.8
00:03:56.36 +49:40:51.0
23:45:02.95 +44:47:30.5
23:54:02.16 +44:33:34.6
23:54:40.83 +44:53:44.4
00:17:32.61 +45:44:45.0
23:35:22.96 +45:57:49.4
23:50:36.77 +47:03:37.0
23:50:20.38 +46:56:39.5
23:39:52.00 +47:45:01.8
00:25:37.48 +47:12:42.8
23:42:09.19 +46:24:30.9
23:34:07.85 +46:20:01.1
########### Completed And-01-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 ####
23:45:02.69 +43:55:27.1
23:50:51.99 +43:04:44.6
23:54:35.24 +43:11:17.5
23:49:13.42 +46:43:10.6
23:44:33.48 +43:14:28.6
00:11:06.94 +46:26:23.7
00:05:25.55 +44:17:04.4
23:39:29.81 +46:54:14.1
23:44:05.99 +49:20:23.0
00:20:21.28 +47:00:00.1
23:44:27.11 +49:42:05.4
23:48:52.06 +42:06:27.2
23:37:29.63 +49:59:55.6
00:14:42.13 +46:51:21.8
23:36:37.63 +45:39:10.0
23:48:36.96 +46:14:52.8
23:41:22.84 +46:52:23.1
23:51:59.05 +49:01:25.1
23:40:11.10 +45:02:54.6
23:48:29.85 +46:16:21.1
23:42:09.74 +44:44:15.5
00:10:16.93 +49:00:00.6
23:39:25.83 +45:44:12.7
23:48:13.28 +47:05:59.6
00:02:09.78 +42:08:05.9
23:40:11.61 +48:47:39.7
23:43:18.01 +43:20:59.1
23:43:32.16 +47:19:20.5
23:36:51.97 +43:17:18.3
23:43:26.90 +47:19:48.7
00:02:11.49 +50:19:51.5
23:43:18.55 +43:20:20.7
23:48:38.73 +43:37:22.6
23:40:08.97 +49:47:07.0
00:09:09.48 +49:47:10.0
00:17:36.20 +50:17:52.3
23:38:10.23 +46:10:53.7
00:01:22.66 +46:44:46.7
23:55:38.15 +48:37:54.5
23:50:22.73 +50:15:37.0
23:38:10.45 +46:47:20.7
23:35:06.16 +47:31:11.1
23:39:17.32 +44:07:56.8
00:03:56.36 +49:40:51.0
23:45:02.95 +44:47:30.5
23:54:02.16 +44:33:34.6
23:54:40.83 +44:53:44.4
00:17:32.61 +45:44:45.0
23:35:22.96 +45:57:49.4
23:50:36.77 +47:03:37.0
23:50:20.38 +46:56:39.5
23:50:34.35 +43:04:29.6
00:25:37.48 +47:12:42.8
23:42:09.19 +46:24:30.9
23:34:07.85 +46:20:01.1
23:39:52.00 +47:45:01.8
###################################################################################
23:45:02.69 +43:55:27.1 -- not an asteroid (will add it to exclusion list)
23:50:51.99 +43:04:44.6 -- not an asteroid (will add it to exclusion list)
23:54:35.24 +43:11:17.5 -- not an asteroid (will add it to exclusion list)
23:49:13.42 +46:43:10.6 -- not an asteroid (will add it to exclusion list)
23:44:33.48 +43:14:28.6 -- not an asteroid (will add it to exclusion list)
00:11:06.94 +46:26:23.7 -- not an asteroid (will add it to exclusion list)
00:05:25.55 +44:17:04.4 -- not an asteroid (will add it to exclusion list)
23:39:29.81 +46:54:14.1 -- not an asteroid (will add it to exclusion list)
23:44:05.99 +49:20:23.0 -- not an asteroid (will add it to exclusion list)
00:20:21.28 +47:00:00.1 -- not an asteroid (will add it to exclusion list)
23:44:27.11 +49:42:05.4 -- not an asteroid (will add it to exclusion list)
23:48:52.06 +42:06:27.2 -- not an asteroid (will add it to exclusion list)
23:37:29.63 +49:59:55.6 -- not an asteroid (will add it to exclusion list)
00:14:42.13 +46:51:21.8 -- not an asteroid (will add it to exclusion list)
23:36:37.63 +45:39:10.0 -- not an asteroid (will add it to exclusion list)
23:48:36.96 +46:14:52.8 -- not an asteroid (will add it to exclusion list)
23:41:22.84 +46:52:23.1 -- not an asteroid (will add it to exclusion list)
23:51:59.05 +49:01:25.1 -- not an asteroid (will add it to exclusion list)
23:40:11.10 +45:02:54.6 -- not an asteroid (will add it to exclusion list)
23:48:29.85 +46:16:21.1 -- not an asteroid (will add it to exclusion list)
23:42:09.74 +44:44:15.5 -- not an asteroid (will add it to exclusion list)
00:10:16.93 +49:00:00.6 -- not an asteroid (will add it to exclusion list)
23:39:25.83 +45:44:12.7 -- not an asteroid (will add it to exclusion list)
23:48:13.28 +47:05:59.6 -- not an asteroid (will add it to exclusion list)
00:02:09.78 +42:08:05.9 -- not an asteroid (will add it to exclusion list)
23:40:11.61 +48:47:39.7 -- not an asteroid (will add it to exclusion list)
23:43:18.01 +43:20:59.1 -- not an asteroid (will add it to exclusion list)
23:43:32.16 +47:19:20.5 -- not an asteroid (will add it to exclusion list)
23:36:51.97 +43:17:18.3 -- not an asteroid (will add it to exclusion list)
23:43:26.90 +47:19:48.7 -- not an asteroid (will add it to exclusion list)
00:02:11.49 +50:19:51.5 -- not an asteroid (will add it to exclusion list)
23:43:18.55 +43:20:20.7 -- not an asteroid (will add it to exclusion list)
23:48:38.73 +43:37:22.6 -- not an asteroid (will add it to exclusion list)
23:40:08.97 +49:47:07.0 -- not an asteroid (will add it to exclusion list)
00:09:09.48 +49:47:10.0 -- not an asteroid (will add it to exclusion list)
00:17:36.20 +50:17:52.3 -- not an asteroid (will add it to exclusion list)
23:38:10.23 +46:10:53.7 -- not an asteroid (will add it to exclusion list)
00:01:22.66 +46:44:46.7 -- not an asteroid (will add it to exclusion list)
23:55:38.15 +48:37:54.5 -- not an asteroid (will add it to exclusion list)
23:50:22.73 +50:15:37.0 -- not an asteroid (will add it to exclusion list)
23:38:10.45 +46:47:20.7 -- not an asteroid (will add it to exclusion list)
23:35:06.16 +47:31:11.1 -- not an asteroid (will add it to exclusion list)
23:39:17.32 +44:07:56.8 -- not an asteroid (will add it to exclusion list)
00:03:56.36 +49:40:51.0 -- not an asteroid (will add it to exclusion list)
23:45:02.95 +44:47:30.5 -- not an asteroid (will add it to exclusion list)
23:54:02.16 +44:33:34.6 -- not an asteroid (will add it to exclusion list)
23:54:40.83 +44:53:44.4 -- not an asteroid (will add it to exclusion list)
00:17:32.61 +45:44:45.0 -- not an asteroid (will add it to exclusion list)
23:35:22.96 +45:57:49.4 -- not an asteroid (will add it to exclusion list)
23:50:36.77 +47:03:37.0 -- not an asteroid (will add it to exclusion list)
23:50:20.38 +46:56:39.5 -- not an asteroid (will add it to exclusion list)
23:50:34.35 +43:04:29.6 -- not an asteroid (will add it to exclusion list)
00:25:37.48 +47:12:42.8 -- not an asteroid (will add it to exclusion list)
23:42:09.19 +46:24:30.9 -- not an asteroid (will add it to exclusion list)
23:34:07.85 +46:20:01.1 -- not an asteroid (will add it to exclusion list)
23:39:52.00 +47:45:01.8 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
00:01:22.66 +46:44:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:02:09.78 +42:08:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:02:11.49 +50:19:51.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:03:56.36 +49:40:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:05:25.55 +44:17:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:09:09.48 +49:47:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:10:16.93 +49:00:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:11:06.94 +46:26:23.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:14:42.13 +46:51:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:17:32.61 +45:44:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:17:36.20 +50:17:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:20:21.28 +47:00:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:25:37.48 +47:12:42.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:34:07.85 +46:20:01.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:35:06.16 +47:31:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:35:22.96 +45:57:49.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:36:37.63 +45:39:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:36:51.97 +43:17:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:37:29.63 +49:59:55.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:38:10.23 +46:10:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:38:10.45 +46:47:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:39:17.32 +44:07:56.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:39:25.83 +45:44:12.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:39:29.81 +46:54:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:39:52.00 +47:45:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:40:08.97 +49:47:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:40:11.10 +45:02:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:40:11.61 +48:47:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:41:22.84 +46:52:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:42:09.19 +46:24:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:42:09.74 +44:44:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:43:18.01 +43:20:59.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:43:18.55 +43:20:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:43:26.90 +47:19:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:43:32.16 +47:19:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:44:05.99 +49:20:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:44:27.11 +49:42:05.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:44:33.48 +43:14:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:45:02.69 +43:55:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:45:02.95 +44:47:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:48:13.28 +47:05:59.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:48:29.85 +46:16:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:48:36.96 +46:14:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:48:38.73 +43:37:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:48:52.06 +42:06:27.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:49:13.42 +46:43:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:50:20.38 +46:56:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:50:22.73 +50:15:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:50:34.35 +43:04:29.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:50:36.77 +47:03:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:50:51.99 +43:04:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:51:59.05 +49:01:25.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:54:02.16 +44:33:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:54:35.24 +43:11:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:54:40.83 +44:53:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:55:38.15 +48:37:54.5 -- 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)
00:01:22.66 +46:44:46.7 -- not a known variable star
00:02:09.78 +42:08:05.9 -- not a known variable star
00:02:11.49 +50:19:51.5 -- not a known variable star
00:03:56.36 +49:40:51.0 -- not a known variable star
00:05:25.55 +44:17:04.4 -- not a known variable star
00:09:09.48 +49:47:10.0 -- not a known variable star
00:10:16.93 +49:00:00.6 -- a known variable star
00:11:06.94 +46:26:23.7 -- not a known variable star
00:14:42.13 +46:51:21.8 -- not a known variable star
00:17:32.61 +45:44:45.0 -- not a known variable star
00:17:36.20 +50:17:52.3 -- not a known variable star
00:20:21.28 +47:00:00.1 -- a known variable star
00:25:37.48 +47:12:42.8 -- a known variable star
23:34:07.85 +46:20:01.1 -- a known variable star
23:35:06.16 +47:31:11.1 -- not a known variable star
23:35:22.96 +45:57:49.4 -- not a known variable star
23:36:37.63 +45:39:10.0 -- a known variable star
23:36:51.97 +43:17:18.3 -- not a known variable star
23:37:29.63 +49:59:55.6 -- not a known variable star
23:38:10.23 +46:10:53.7 -- not a known variable star
23:38:10.45 +46:47:20.7 -- a known variable star
23:39:17.32 +44:07:56.8 -- not a known variable star
23:39:25.83 +45:44:12.7 -- not a known variable star
23:39:29.81 +46:54:14.1 -- not a known variable star
23:39:52.00 +47:45:01.8 -- a known variable star
23:40:08.97 +49:47:07.0 -- not a known variable star
23:40:11.10 +45:02:54.6 -- not a known variable star
23:40:11.61 +48:47:39.7 -- a known variable star
23:41:22.84 +46:52:23.1 -- not a known variable star
23:42:09.19 +46:24:30.9 -- a known variable star
23:42:09.74 +44:44:15.5 -- not a known variable star
23:43:18.01 +43:20:59.1 -- not a known variable star
23:43:18.55 +43:20:20.7 -- not a known variable star
23:43:26.90 +47:19:48.7 -- not a known variable star
23:43:32.16 +47:19:20.5 -- not a known variable star
23:44:05.99 +49:20:23.0 -- a known variable star
23:44:27.11 +49:42:05.4 -- not a known variable star
23:44:33.48 +43:14:28.6 -- not a known variable star
23:45:02.69 +43:55:27.1 -- a known variable star
23:45:02.95 +44:47:30.5 -- not a known variable star
23:48:13.28 +47:05:59.6 -- not a known variable star
23:48:29.85 +46:16:21.1 -- not a known variable star
23:48:36.96 +46:14:52.8 -- not a known variable star
23:48:38.73 +43:37:22.6 -- a known variable star
23:48:52.06 +42:06:27.2 -- a known variable star
23:49:13.42 +46:43:10.6 -- not a known variable star
23:50:20.38 +46:56:39.5 -- not a known variable star
23:50:22.73 +50:15:37.0 -- not a known variable star
23:50:34.35 +43:04:29.6 -- a known variable star
23:50:36.77 +47:03:37.0 -- not a known variable star
23:50:51.99 +43:04:44.6 -- a known variable star
23:51:59.05 +49:01:25.1 -- not a known variable star
23:54:02.16 +44:33:34.6 -- not a known variable star
23:54:35.24 +43:11:17.5 -- a known variable star
23:54:40.83 +44:53:44.4 -- not a known variable star
23:55:38.15 +48:37:54.5 -- not a known variable star
Found 40 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
56 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 56 (excluding asteroids and hot pixels, 40 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)2461149.94236278 -observatory V36
00:26:03.19 -00:02:51.8 Mercury (-0.1mag)
03:25:35.77 +19:06:02.5 Venus (-3.9mag)
00:27:36.91 +01:56:15.3 Mars (1.2mag)
07:14:15.44 +22:43:30.5 Jupiter (-2.1mag)
00:30:42.43 +00:58:27.5 Saturn (0.9mag)
03:48:25.94 +19:49:49.2 Uranus (5.8mag)
00:11:17.17 -00:12:34.3 Neptune (7.8mag)
20:33:53.63 -22:52:48.1 Pluto (14.5mag)
03:31:47.14 +23:20:30.2 Moon (-8.8mag)
-rw-r--r-- 1 apache apache 362 Apr 19 05:40 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461149.94236278:
07:14:11.24 +22:43:41.4 Io (5.8mag)
07:14:16.11 +22:43:32.0 Europa (5.9mag)
07:13:57.23 +22:44:11.4 Ganymede (5.4mag)
07:14:27.78 +22:42:55.9 Callisto (6.6mag)
07:17:26.27 +22:29:35.1 Himalia (15.4mag)
07:14:15.54 +22:43:28.1 Thebe (16.2mag)
07:17:41.86 +22:59:55.0 Elara (17.3mag)
07:13:22.40 +23:21:42.8 Pasiphae (17.4mag)
07:22:30.43 +22:41:51.2 Carme (18.5mag)
00:30:33.19 +00:58:47.6 Titan (8.8mag)
00:30:40.15 +00:58:43.3 Rhea (10.1mag)
00:30:17.33 +00:58:03.8 Iapetus (11.5mag)
00:30:37.47 +00:58:55.3 Hyperion (14.8mag)
00:32:16.53 +01:06:53.0 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 19 05:40 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461149.94236278:
15:51:36.43 -18:36:15.6 JWST
16:45:49.75 +46:33:42.0 Chandra
20:11:51.31 +24:20:37.4 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 19 05:40 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461149.94236278 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:53:16.41 -28:59:10.6 13.9mag P/2010 H2 (Vales)
05:09:15.73 -69:30:08.8 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:33:13.47 +31:27:41.4 17.2mag C/2017 K2 (PANSTARRS)
17:30:01.86 +10:57:06.0 17.6mag C/2021 G2 (ATLAS)
23:11:05.76 +29:22:08.8 17.1mag C/2022 E2 (ATLAS)
04:33:16.51 +26:07:48.1 16.0mag C/2022 N2 (PANSTARRS)
09:04:14.46 +32:01:48.2 16.2mag C/2022 QE78 (ATLAS)
08:31:39.89 +00:12:15.2 17.4mag C/2022 R6 (PANSTARRS)
18:52:50.55 +18:49:04.7 17.6mag C/2023 A3 (Tsuchinshan-ATLAS)
15:39:30.67 -11:28:15.3 17.5mag P/2023 B1 (PANSTARRS)
09:06:08.52 -11:20:27.4 17.7mag C/2023 F3 (ATLAS)
21:57:31.84 +63:06:50.1 17.5mag C/2023 H5 (Lemmon)
19:16:00.92 -03:47:46.5 14.1mag C/2023 R1 (PANSTARRS)
21:23:28.24 +86:23:39.7 17.8mag C/2023 X2 (Lemmon)
06:19:40.46 +63:30:06.9 17.2mag C/2024 A1 (ATLAS)
05:20:31.07 +19:23:30.4 11.3mag C/2024 E1 (Wierzchos)
16:16:59.53 +06:57:07.6 17.4mag C/2024 G6 (ATLAS)
20:21:41.34 +16:13:13.4 14.6mag C/2024 J3 (ATLAS)
03:29:29.46 -21:52:08.5 16.3mag C/2024 T5 (ATLAS)
05:19:40.61 +44:27:08.0 17.7mag C/2025 J1 (Borisov)
13:24:40.07 +47:30:09.2 15.3mag C/2025 L1 (ATLAS)
03:30:48.95 -26:45:39.7 17.9mag C/2025 Q3 (ATLAS)
00:21:56.30 +16:48:57.8 8.1mag C/2025 R3 (PANSTARRS)
12:52:38.42 +03:13:00.1 17.4mag C/2025 Y1 (ATLAS)
03:53:17.34 +02:18:40.6 14.2mag C/2026 A1 (MAPS)
00:09:11.83 +37:49:45.1 14.7mag C/2026 B2 (Sun-Gao)
18:49:37.34 -09:31:57.5 11.6mag 10P/Tempel
14:55:35.68 +02:49:55.1 14.3mag 24P/Schaumasse
11:01:56.46 -01:25:10.1 15.7mag 29P/Schwassmann-Wachmann
10:37:33.97 -03:50:18.3 17.0mag 43P/Wolf-Harrington
01:54:00.89 +18:04:13.9 17.3mag 47P/Ashbrook-Jackson
07:17:12.90 +36:15:53.7 17.0mag 63P/Wild
23:33:24.47 -11:02:32.7 15.7mag 65P/Gunn
04:12:33.44 +22:24:43.8 15.9mag 76P/West-Kohoutek-Ikemura
01:13:13.36 +08:54:04.7 14.3mag 78P/Gehrels
23:13:18.59 -08:22:21.6 14.7mag 88P/Howell
02:20:14.13 +21:32:39.6 15.1mag 93P/Lovas
05:01:23.59 +32:27:49.7 16.2mag 123P/West-Hartley
08:32:34.17 +36:46:26.4 16.2mag 124P/Mrkos
02:38:33.90 +14:45:00.3 16.4mag 128P/Shoemaker-Holt
02:54:18.70 +14:54:18.3 17.5mag 131P/Mueller
01:44:25.66 +14:22:41.2 10.5mag 141P/Machholz
01:52:49.58 +06:09:25.8 10.5mag 141P-A/Machholz
00:36:35.25 +01:57:50.0 12.4mag 141P-D/Machholz
02:23:22.13 +07:54:42.2 17.9mag 141P-I/Machholz
01:12:00.86 +00:12:38.7 15.0mag 162P/SidingSpring
14:45:20.41 +00:15:51.4 17.8mag 210P/Christensen
21:48:33.93 -10:37:27.2 17.7mag 218P/LINEAR
17:17:11.10 -13:30:55.1 16.1mag 235P/LINEAR
05:41:58.50 +34:56:33.4 16.8mag 240P/NEAT
07:40:16.10 -04:48:16.8 17.8mag 242P/Spahr
22:25:31.43 -20:02:35.5 17.8mag 260P/McNaught
02:05:17.08 +21:19:19.1 18.0mag 295P/LINEAR
15:41:13.58 +07:12:35.7 17.5mag 391P/Kowalski
07:35:35.69 +21:22:20.9 17.7mag 450P/LONEOS
05:40:56.96 +44:49:52.5 17.5mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.8K Apr 19 05:40 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 05:40 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 05:40 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
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
19:45:48.257 -49:40:35.86 AT 2026jin 2026-04-12.35 18.142
-rw-r--r-- 1 apache apache 30K Apr 19 05:40 tns_transients_list.txt
