This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe
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 06.4781* 23 45 02.30 +43 55 29.4 10.4 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
EY And,2461136.9781,10.39,0.05,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
EY And 20260406.4781 10.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.4781* 00 10 55.01 +48 15 31.7 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
LD 323,2461136.9781,10.69,0.05,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
LD 323 20260406.4781 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 06.4781* 00 22 05.07 +44 08 44.0 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 3656996,2461136.9781,10.19,0.05,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
NSVS 3656996 20260406.4781 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 06.4781* 23 43 33.28 +50 00 45.0 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1943568466332031104,2461136.9781,12.19,0.05,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 1943568466332031104 20260406.4781 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 06.4781* 23 51 51.58 +48 26 38.5 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J357.9705+48.4419,2461136.9781,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J357.9705+48.4419 20260406.4781 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.4781* 23 36 39.60 +42 43 33.5 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J354.1786+42.7293,2461136.9781,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J354.1786+42.7293 20260406.4781 11.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.4781* 23 37 29.46 +49 59 56.1 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1943698346142347136,2461136.9781,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1943698346142347136 20260406.4781 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.4781* 00 03 07.80 +50 05 56.9 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 393901002723435648,2461136.9781,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 393901002723435648 20260406.4781 11.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.4781* 00 14 41.96 +46 51 20.8 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 392207548658221312,2461136.9781,11.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 392207548658221312 20260406.4781 11.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.4781* 23 37 21.30 +46 30 57.3 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1939162036042408576,2461136.9781,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1939162036042408576 20260406.4781 11.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.4781* 23 48 42.61 +46 14 34.8 10.6 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1927283771411171200,2461136.9781,10.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1927283771411171200 20260406.4781 10.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.4781* 23 58 41.26 +48 31 40.3 10.5 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1939623349887934336,2461136.9781,10.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1939623349887934336 20260406.4781 10.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.4781* 23 57 30.24 +48 17 26.3 9.5 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1939610705511944064,2461136.9781,9.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1939610705511944064 20260406.4781 9.46CV 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 06.4781* 23 50 51.89 +43 04 44.7 9.9 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
EZ And,2461136.9781,9.87,0.05,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
EZ And 20260406.4781 9.87CV 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 06.4781* 23 41 22.75 +46 52 23.8 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1939240926002369536,2461136.9781,10.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1939240926002369536 20260406.4781 10.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.4781* 00 07 52.40 +44 04 40.8 10.5 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 386261080537712256,2461136.9781,10.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 386261080537712256 20260406.4781 10.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.4781* 23 51 58.92 +49 01 24.8 10.7 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1940551268987081856,2461136.9781,10.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1940551268987081856 20260406.4781 10.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.4781* 23 40 11.01 +45 02 53.6 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1926756143267842048,2461136.9781,10.87,0.05,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
Gaia DR3 1926756143267842048 20260406.4781 10.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.4781* 23 34 59.81 +46 03 42.4 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1937601657244802688,2461136.9781,11.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1937601657244802688 20260406.4781 11.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.4781* 00 06 03.42 +49 37 34.6 10.9 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 393829190871939328,2461136.9781,10.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 393829190871939328 20260406.4781 10.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.4781* 23 48 29.60 +46 16 21.9 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1927284797904773120,2461136.9781,10.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1927284797904773120 20260406.4781 10.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.4781* 23 42 09.57 +44 44 15.8 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1926630524064281088,2461136.9781,11.07,0.05,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 1926630524064281088 20260406.4781 11.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.4781* 00 12 42.80 +44 18 43.0 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J001245.77+441906.0,2461136.9781,10.74,0.05,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
ASASSN-V J001245.77+441906.0 20260406.4781 10.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.4781* 00 10 16.89 +49 00 01.5 11.1 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 393561876404915840,2461136.9781,11.07,0.05,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 393561876404915840 20260406.4781 11.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.4781* 00 05 31.30 +48 29 22.4 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 393374787630869888,2461136.9781,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 393374787630869888 20260406.4781 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.4781* 00 15 45.59 +45 30 23.6 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 386067914386294656,2461136.9781,10.94,0.05,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
Gaia DR3 386067914386294656 20260406.4781 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 06.4781* 00 01 37.73 +44 41 34.4 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 385039385680155904,2461136.9781,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 385039385680155904 20260406.4781 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.4781* 23 50 37.84 +47 30 33.5 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J357.6529+47.5164,2461136.9781,11.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J357.6529+47.5164 20260406.4781 11.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.4781* 23 45 20.72 +44 17 43.0 11.2 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.9781,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.4781 11.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.4781* 23 43 30.36 +47 20 00.6 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.9781,11.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.4781 11.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.4781* 23 52 55.93 +48 28 15.9 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J358.2339+48.4708,2461136.9781,11.27,0.05,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 J358.2339+48.4708 20260406.4781 11.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.4781* 23 35 37.75 +43 44 51.8 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1924982734091052288,2461136.9781,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1924982734091052288 20260406.4781 11.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.4781* 23 39 25.53 +45 44 14.1 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.9781,11.38,0.05,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
target 20260406.4781 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 06.4781* 00 16 05.85 +46 59 40.2 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.9781,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.4781 11.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.4781* 23 48 13.24 +47 05 59.1 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J357.0571+47.0984,2461136.9781,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J357.0571+47.0984 20260406.4781 11.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.4781* 23 55 59.49 +48 12 26.6 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1939590467625105920,2461136.9781,11.39,0.05,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
Gaia DR3 1939590467625105920 20260406.4781 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 06.4781* 23 54 25.47 +48 54 43.0 11.5 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J358.5960+48.9077,2461136.9781,11.54,0.05,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
ATO J358.5960+48.9077 20260406.4781 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 06.4781* 23 44 56.16 +50 07 12.0 11.5 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J356.2264+50.1141,2461136.9781,11.54,0.05,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
ATO J356.2264+50.1141 20260406.4781 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 06.4781* 00 02 09.82 +42 08 07.2 11.2 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.9781,11.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.4781 11.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.4781* 00 10 38.93 +48 37 01.3 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.9781,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.4781 11.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.4781* 23 40 11.38 +48 47 40.4 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1940343186409018112,2461136.9781,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1940343186409018112 20260406.4781 11.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.4781* 23 57 14.32 +45 56 53.5 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1926384370896570112,2461136.9781,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1926384370896570112 20260406.4781 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.4781* 00 18 30.42 +43 59 38.6 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J004.6157+43.9987,2461136.9781,11.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J004.6157+43.9987 20260406.4781 11.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.4781* 00 05 48.54 +45 47 23.2 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.9781,11.49,0.05,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 20260406.4781 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 06.4781* 23 43 31.91 +47 19 18.6 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.9781,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.4781 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.4781* 23 43 03.30 +49 07 40.0 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J355.7497+49.1276,2461136.9781,11.74,0.05,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
ATO J355.7497+49.1276 20260406.4781 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 06.4781* 00 09 56.46 +46 22 42.7 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.9781,11.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.4781 11.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.4781* 00 01 42.40 +46 36 22.1 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J000.4293+46.6268,2461136.9781,11.70,0.05,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
ATO J000.4293+46.6268 20260406.4781 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 06.4781* 23 57 42.49 +48 23 29.1 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J359.4230+48.3956,2461136.9781,11.94,0.05,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
ATO J359.4230+48.3956 20260406.4781 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.4781* 00 01 31.96 +47 56 37.5 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.9781,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.4781 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.4781* 23 43 18.08 +43 21 01.5 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.9781,11.69,0.05,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 20260406.4781 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 06.4781* 23 58 57.37 +44 34 56.5 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1923015707786968704,2461136.9781,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1923015707786968704 20260406.4781 11.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.4781* 23 46 58.69 +48 49 35.7 11.9 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1940577897784457856,2461136.9781,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1940577897784457856 20260406.4781 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.4781* 00 10 08.09 +50 09 19.5 11.9 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J002.5348+50.1712,2461136.9781,11.95,0.05,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
ATO J002.5348+50.1712 20260406.4781 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.4781* 23 58 27.09 +48 35 38.7 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1939636440956849280,2461136.9781,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1939636440956849280 20260406.4781 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.4781* 23 45 46.47 +48 26 37.5 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461136.9781,12.12,0.05,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
VARIABLE_NAME 20260406.4781 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 06.4781* 00 01 22.58 +46 44 47.0 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.9781,12.09,0.05,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 20260406.4781 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 06.4781* 23 38 09.87 +46 10 52.9 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1939093763243856896,2461136.9781,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1939093763243856896 20260406.4781 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.4781* 23 45 02.59 +44 47 30.5 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.9781,12.27,0.05,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
target 20260406.4781 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 06.4781* 23 54 39.78 +49 17 01.7 12.3 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1940649572198432128,2461136.9781,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1940649572198432128 20260406.4781 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.4781* 23 46 42.47 +44 27 24.3 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.9781,12.29,0.05,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
target 20260406.4781 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 06.4781* 00 21 48.81 +44 52 17.8 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0021489+445219,2461136.9781,10.70,0.05,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
NSVS J0021489+445219 20260406.4781 10.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.4781* 00 19 50.27 +47 42 36.6 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0960 Cas,2461136.9781,11.31,0.05,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
V0960 Cas 20260406.4781 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 06.4781* 23 50 36.09 +47 31 26.5 10.4 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J357.6529+47.5164,2461136.9781,10.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J357.6529+47.5164 20260406.4781 10.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.4781* 23 54 35.04 +43 11 16.7 10.4 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2354350+431115,2461136.9781,10.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2354350+431115 20260406.4781 10.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.4781* 23 34 07.49 +46 20 03.2 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0339 And,2461136.9781,11.32,0.05,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
V0339 And 20260406.4781 11.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.4781* 23 39 51.84 +47 45 01.3 11.2 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
EX And,2461136.9781,11.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
EX And 20260406.4781 11.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## 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: 2461136.97851565 06.04.2026 11:28:53.752 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 5
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: 5 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): 17156
Objects passed selection criteria: 17061
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 11111.8
Average stars matched: 10367 (93.2976 %)
Memory usage VmPeak: 121812 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 6 07:15:01 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: 2461136.97851565 06.04.2026 11:28:53.752 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 101
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: 78 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): 113103
Objects passed selection criteria: 112744
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 78108.5
Average stars matched: 71656 (91.7391 %)
Memory usage VmPeak: 2859228 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 6 07:17:40 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_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.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_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.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: 2461136.97768021
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
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_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits exists and is non-empty
Saving wcs_fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits to local_wcs_cache/
'wcs_fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits' -> 'local_wcs_cache/wcs_fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits'
wcs_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.fits exists and is non-empty
Saving wcs_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.fits to local_wcs_cache/
'wcs_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.fits' -> 'local_wcs_cache/wcs_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.fits'
The image scale is 5.80"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.7"
###################################
# 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 00:00:19.324 +46:01:25.70
Angular distance between the image centers 0.0551 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# 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 00:00:16.733 +46:00:41.75
Angular distance between the image centers 0.0436 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 00:00:19.324 +46:01:25.70
Second-epoch second image center 00:00:16.733 +46:00:41.75
Angular distance between the image centers 0.01433 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.OANrYPNr0P
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.sAfo7eW55a
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_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits &> /tmp/tmp.3ZwFZGPoBC
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.fits &> /tmp/tmp.2Kd7VRwa0l
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.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 4 candidate transients before the final filtering. (Hard limit: 3000)
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
2.5 pix fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits
2.5 pix fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.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
13.6 mag. fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits
13.5 mag. fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.fits
All-image limiting magnitude estimate: 13.5 (SNR ) 10.9 (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.OANrYPNr0P (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_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/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...
WARNING: 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...
WARNING: 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
WARNING: 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"
WARNING: 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.sAfo7eW55a (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_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/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...
WARNING: 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...
WARNING: 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
WARNING: 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"
WARNING: 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.3ZwFZGPoBC (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_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.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_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits
WCS_IMAGE_NAME=wcs_fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits
WCS-calibrated image found: wcs_fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits
Checking if the catalog wcs_fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits.cat corresponding to the image wcs_fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits alredy exist and is non-empty...
Catalog wcs_fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits.cat corresponding to the image wcs_fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.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_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits
WCS catalog name: wcs_fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=578, passed=7339
Got 7339 stars (including 6756 good ones) from the SExtractor catalog wcs_fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits.cat
util/solve_plate_with_UCAC5 got 7339 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 347.6243 through 0 to 12.2320, gap 12.2320 to 347.6243
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.2 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...
WARNING: Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 912 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 7156 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
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 347.6244 through 0 to 12.2324, gap 12.2324 to 347.6244
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.2 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
WARNING: Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 7156 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
WARNING: Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 7156 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
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_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits -region wcs_fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.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.2Kd7VRwa0l (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_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.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_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.fits
WCS_IMAGE_NAME=wcs_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.fits
WCS-calibrated image found: wcs_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.fits
Checking if the catalog wcs_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.fits.cat corresponding to the image wcs_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.fits alredy exist and is non-empty...
Catalog wcs_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.fits.cat corresponding to the image wcs_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.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_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.fits
WCS catalog name: wcs_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=553, passed=6949
Got 6949 stars (including 6390 good ones) from the SExtractor catalog wcs_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.fits.cat
util/solve_plate_with_UCAC5 got 6949 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 347.6242 through 0 to 12.2320, gap 12.2320 to 347.6242
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.2 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...
WARNING: Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 911 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 6744 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
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 347.6243 through 0 to 12.2323, gap 12.2323 to 347.6243
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.2 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
WARNING: Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 6745 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
WARNING: Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 6770 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
Excluding outliers - 935 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_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.fits -region wcs_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.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_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/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_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/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_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/wcs_fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits'
Saving fully-calibrated image wcs_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/wcs_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.fits'
Preparing the HTML report for the field And-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out31958.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out07730.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15590.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31852.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 4s
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 31852_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 31852_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31958_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
The candidate 31958_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495 did not pass the final checks
**** FOUND 00:12:06.69 +48:12:20.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.41, MAG_FAINT_SEARCH_LIMIT=11.39)GAIADR2_OUTPUT=# 2.357 393128015988361216 003.02811802971 +48.20624549159 9.0607 7.6189 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.357#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07730_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 07730_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15590_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 15590_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 6s
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 ####
00:10:55.01 +48:15:31.7
00:22:05.07 +44:08:44.0
23:45:02.30 +43:55:29.4
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_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.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_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.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_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits
Creating symlink local_wcs_cache/wcs_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.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_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits exists and is non-empty
wcs_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.fits exists and is non-empty
The image scale is 5.80"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.7"
###################################
# 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 00:00:19.324 +46:01:25.70
Angular distance between the image centers 0.0551 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# 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 00:00:16.733 +46:00:41.75
Angular distance between the image centers 0.0436 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 00:00:19.324 +46:01:25.70
Second-epoch second image center 00:00:16.733 +46:00:41.75
Angular distance between the image centers 0.01433 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.tFrlCzeYuq
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.XqSL8dRvXh
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_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits &> /tmp/tmp.Dj6crqaTCX
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.fits &> /tmp/tmp.6XJE7VsxXe
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.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 81 candidate transients before the final filtering. (Hard limit: 3000)
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
2.3 pix fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits
2.2 pix fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.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
12.4 mag. fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits
12.4 mag. fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.fits
All-image limiting magnitude estimate: 12.4 (SNR ) 11.9 (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.tFrlCzeYuq (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_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/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...
WARNING: 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...
WARNING: 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
WARNING: 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"
WARNING: 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.XqSL8dRvXh (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_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/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...
WARNING: 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...
WARNING: 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
WARNING: 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"
WARNING: 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.Dj6crqaTCX (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_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.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_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits
WCS_IMAGE_NAME=wcs_fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits
WCS-calibrated image found: wcs_fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits
Checking if the catalog wcs_fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits.cat corresponding to the image wcs_fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits alredy exist and is non-empty...
Catalog wcs_fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits.cat corresponding to the image wcs_fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.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_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits
WCS catalog name: wcs_fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=3324, passed=53046
Got 53046 stars (including 49655 good ones) from the SExtractor catalog wcs_fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits.cat
util/solve_plate_with_UCAC5 got 53046 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 347.5471 through 0 to 12.2318, gap 12.2318 to 347.5471
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.1 to 51.3)
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 914 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 51938 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
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 347.5470 through 0 to 12.2321, gap 12.2321 to 347.5470
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.1 to 51.3)
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 51935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
WARNING: Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 51935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
Excluding outliers - 938 stars left (next iteration limit 1031)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits -region wcs_fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.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.6XJE7VsxXe (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_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.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_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.fits
WCS_IMAGE_NAME=wcs_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.fits
WCS-calibrated image found: wcs_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.fits
Checking if the catalog wcs_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.fits.cat corresponding to the image wcs_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.fits alredy exist and is non-empty...
Catalog wcs_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.fits.cat corresponding to the image wcs_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.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_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.fits
WCS catalog name: wcs_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=3239, passed=51450
Got 51450 stars (including 48140 good ones) from the SExtractor catalog wcs_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.fits.cat
util/solve_plate_with_UCAC5 got 51450 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 347.5471 through 0 to 12.2390, gap 12.2390 to 347.5471
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.1 to 51.3)
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 909 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.74"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 50216 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 347.5462 through 0 to 12.2392, gap 12.2392 to 347.5462
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.1 to 51.3)
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 50221 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
WARNING: Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 50297 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
Excluding outliers - 938 stars left (next iteration limit 1030)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.fits -region wcs_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.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_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/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_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/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_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.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_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/wcs_fd_And-01-Q2b1x1_2026-04-06_06-27-41_20.00sec_-5.00C_LIGHT_0494.fits
Saving fully-calibrated image wcs_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.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_2026-04-06_CI_And-01-Q2b1x1_062941_TTUQ2b1x1_23341_SAG2xXqe/wcs_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495.fits
Preparing the HTML report for the field And-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out162870.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out118010.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161709.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161713.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161723.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161724.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161725.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161728.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161732.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161734.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161735.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out163170.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out164010.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out164380.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out165842.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out166061.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167000.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167072.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167112.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167466.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167674.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167679.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168157.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168328.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168364.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168458.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168557.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168650.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168750.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168919.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168969.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168970.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169990.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out170122.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out170174.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out170295.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out170506.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out170617.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out170635.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out170899.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out170952.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out171170.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out171643.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out171735.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out172138.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out172492.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out172526.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out172566.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out172636.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173015.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173109.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out174274.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175338.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175365.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175509.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175535.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175992.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176138.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176280.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176454.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52886.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57324.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out59955.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77205.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out91789.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 88s
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: 34s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 161709_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 161709_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 161713_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 161713_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 161723_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 161723_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 161724_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 161724_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 161725_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 161725_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 161728_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 161728_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 161732_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 161732_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 161734_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 161734_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 161735_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 161735_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 162827_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
The candidate 162827_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495 did not pass the final checks
**** FOUND 23:45:02.56 +43:55:27.3 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 162870_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
The candidate 162870_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495 did not pass the final checks
**** FOUND 00:12:06.64 +48:12:20.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.09, MAG_FAINT_SEARCH_LIMIT=10.07)GAIADR2_OUTPUT=# 2.348 393128015988361216 003.02811802971 +48.20624549159 9.0607 7.6189 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.348#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 163170_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 163170_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 164010_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 164010_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 164380_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 164380_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 164859_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
The candidate 164859_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495 did not pass the final checks
**** FOUND 00:16:23.23 +43:36:55.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 165631_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
The candidate 165631_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495 did not pass the final checks
**** FOUND 23:40:14.79 +44:20:46.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 165842_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 165842_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166058_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
The candidate 166058_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495 did not pass the final checks
**** FOUND 23:37:22.43 +46:26:35.9 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166061_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 166061_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166159_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
The candidate 166159_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495 did not pass the final checks
**** FOUND 00:16:27.78 +43:36:53.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166468_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
The candidate 166468_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495 did not pass the final checks
**** FOUND 23:38:00.14 +46:13:36.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166787_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
The candidate 166787_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495 did not pass the final checks
**** FOUND 23:38:07.27 +46:11:05.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167000_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 167000_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167072_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 167072_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167112_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 167112_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167466_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 167466_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167674_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 167674_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167679_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 167679_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167972_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
The candidate 167972_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495 did not pass the final checks
**** FOUND 23:38:16.67 +43:17:05.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168059_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
The candidate 168059_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495 did not pass the final checks
**** FOUND 23:37:36.91 +44:27:15.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168157_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 168157_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168285_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
The candidate 168285_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495 did not pass the final checks
**** FOUND 23:38:12.46 +43:18:00.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168328_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 168328_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168364_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 168364_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168458_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 168458_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168557_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 168557_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168650_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 168650_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168750_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 168750_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168919_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 168919_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168969_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 168969_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168970_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 168970_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 169990_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 169990_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170122_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 170122_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170174_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 170174_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170180_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
The candidate 170180_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495 did not pass the final checks
**** FOUND 23:37:41.39 +44:25:26.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170247_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
The candidate 170247_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495 did not pass the final checks
**** FOUND 00:11:59.93 +48:07:14.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170295_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 170295_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170506_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 170506_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170617_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 170617_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170635_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 170635_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170899_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 170899_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170952_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 170952_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171170_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 171170_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171643_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 171643_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171735_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 171735_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 172138_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 172138_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 172492_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 172492_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 172526_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 172526_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 172566_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 172566_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 172636_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 172636_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 172862_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
The candidate 172862_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495 did not pass the final checks
**** FOUND 23:52:01.78 +50:05:59.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173015_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 173015_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173109_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 173109_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 174274_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 174274_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 175338_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 175338_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 175365_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 175365_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 175509_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 175509_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 175535_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 175535_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 175992_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 175992_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 176138_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 176138_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 176280_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 176280_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 176454_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 176454_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46096_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
The candidate 46096_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495 did not pass the final checks
**** FOUND 00:10:54.94 +48:15:31.9 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137188_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
The candidate 137188_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495 did not pass the final checks
**** FOUND 00:22:04.89 +44:08:43.4 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 91789_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 91789_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52886_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 52886_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 59955_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 59955_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118010_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 118010_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 77205_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 77205_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 117622_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
The candidate 117622_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495 did not pass the final checks
**** FOUND 00:04:30.64 +42:07:13.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57324_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
Preparing report for the candidate 57324_fd_And-01-Q2b1x1_2026-04-06_06-28-53_20.00sec_-4.90C_LIGHT_0495
make_report_in_HTML.sh Phase 2 (HTML assembly): 4s
make_report_in_HTML.sh TOTAL: 126s
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 ####
00:10:55.01 +48:15:31.7
00:22:05.07 +44:08:44.0
23:45:02.30 +43:55:29.4
23:54:35.04 +43:11:16.7
23:43:33.28 +50:00:45.0
23:51:51.58 +48:26:38.5
23:36:39.60 +42:43:33.5
23:37:29.46 +49:59:56.1
00:03:07.80 +50:05:56.9
00:14:41.96 +46:51:20.8
23:37:21.30 +46:30:57.3
23:48:42.61 +46:14:34.8
23:58:41.26 +48:31:40.3
23:57:30.24 +48:17:26.3
23:50:51.89 +43:04:44.7
23:41:22.75 +46:52:23.8
00:07:52.40 +44:04:40.8
23:51:58.92 +49:01:24.8
23:40:11.01 +45:02:53.6
23:34:59.81 +46:03:42.4
00:06:03.42 +49:37:34.6
23:48:29.60 +46:16:21.9
23:42:09.57 +44:44:15.8
00:12:42.80 +44:18:43.0
00:10:16.89 +49:00:01.5
00:05:31.30 +48:29:22.4
00:15:45.59 +45:30:23.6
00:01:37.73 +44:41:34.4
23:50:37.84 +47:30:33.5
23:45:20.72 +44:17:43.0
23:43:30.36 +47:20:00.6
23:52:55.93 +48:28:15.9
23:35:37.75 +43:44:51.8
23:39:25.53 +45:44:14.1
00:16:05.85 +46:59:40.2
23:48:13.24 +47:05:59.1
23:55:59.49 +48:12:26.6
23:54:25.47 +48:54:43.0
23:44:56.16 +50:07:12.0
00:02:09.82 +42:08:07.2
00:10:38.93 +48:37:01.3
23:40:11.38 +48:47:40.4
23:57:14.32 +45:56:53.5
00:18:30.42 +43:59:38.6
00:05:48.54 +45:47:23.2
23:43:31.91 +47:19:18.6
23:43:03.30 +49:07:40.0
00:09:56.46 +46:22:42.7
00:01:42.40 +46:36:22.1
23:57:42.49 +48:23:29.1
00:01:31.96 +47:56:37.5
23:43:18.08 +43:21:01.5
23:58:57.37 +44:34:56.5
23:46:58.69 +48:49:35.7
00:10:08.09 +50:09:19.5
23:58:27.09 +48:35:38.7
23:45:46.47 +48:26:37.5
00:01:22.58 +46:44:47.0
23:38:09.87 +46:10:52.9
23:45:02.59 +44:47:30.5
23:54:39.78 +49:17:01.7
23:46:42.47 +44:27:24.3
00:19:50.27 +47:42:36.6
23:39:51.84 +47:45:01.3
23:50:36.09 +47:31:26.5
23:34:07.49 +46:20:03.2
00:21:48.81 +44:52:17.8
########### 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 ####
23:45:02.30 +43:55:29.4
00:10:55.01 +48:15:31.7
00:22:05.07 +44:08:44.0
23:43:33.28 +50:00:45.0
23:51:51.58 +48:26:38.5
23:36:39.60 +42:43:33.5
23:37:29.46 +49:59:56.1
00:03:07.80 +50:05:56.9
00:14:41.96 +46:51:20.8
23:37:21.30 +46:30:57.3
23:48:42.61 +46:14:34.8
23:58:41.26 +48:31:40.3
23:57:30.24 +48:17:26.3
23:50:51.89 +43:04:44.7
23:41:22.75 +46:52:23.8
00:07:52.40 +44:04:40.8
23:51:58.92 +49:01:24.8
23:40:11.01 +45:02:53.6
23:34:59.81 +46:03:42.4
00:06:03.42 +49:37:34.6
23:48:29.60 +46:16:21.9
23:42:09.57 +44:44:15.8
00:12:42.80 +44:18:43.0
00:10:16.89 +49:00:01.5
00:05:31.30 +48:29:22.4
00:15:45.59 +45:30:23.6
00:01:37.73 +44:41:34.4
23:50:37.84 +47:30:33.5
23:45:20.72 +44:17:43.0
23:43:30.36 +47:20:00.6
23:52:55.93 +48:28:15.9
23:35:37.75 +43:44:51.8
23:39:25.53 +45:44:14.1
00:16:05.85 +46:59:40.2
23:48:13.24 +47:05:59.1
23:55:59.49 +48:12:26.6
23:54:25.47 +48:54:43.0
23:44:56.16 +50:07:12.0
00:02:09.82 +42:08:07.2
00:10:38.93 +48:37:01.3
23:40:11.38 +48:47:40.4
23:57:14.32 +45:56:53.5
00:18:30.42 +43:59:38.6
00:05:48.54 +45:47:23.2
23:43:31.91 +47:19:18.6
23:43:03.30 +49:07:40.0
00:09:56.46 +46:22:42.7
00:01:42.40 +46:36:22.1
23:57:42.49 +48:23:29.1
00:01:31.96 +47:56:37.5
23:43:18.08 +43:21:01.5
23:58:57.37 +44:34:56.5
23:46:58.69 +48:49:35.7
00:10:08.09 +50:09:19.5
23:58:27.09 +48:35:38.7
23:45:46.47 +48:26:37.5
00:01:22.58 +46:44:47.0
23:38:09.87 +46:10:52.9
23:45:02.59 +44:47:30.5
23:54:39.78 +49:17:01.7
23:46:42.47 +44:27:24.3
00:21:48.81 +44:52:17.8
00:19:50.27 +47:42:36.6
23:50:36.09 +47:31:26.5
23:54:35.04 +43:11:16.7
23:34:07.49 +46:20:03.2
23:39:51.84 +47:45:01.3
###################################################################################
23:45:02.30 +43:55:29.4 -- not an asteroid (will add it to exclusion list)
00:10:55.01 +48:15:31.7 -- not an asteroid (will add it to exclusion list)
00:22:05.07 +44:08:44.0 -- not an asteroid (will add it to exclusion list)
23:43:33.28 +50:00:45.0 -- not an asteroid (will add it to exclusion list)
23:51:51.58 +48:26:38.5 -- not an asteroid (will add it to exclusion list)
23:36:39.60 +42:43:33.5 -- not an asteroid (will add it to exclusion list)
23:37:29.46 +49:59:56.1 -- not an asteroid (will add it to exclusion list)
00:03:07.80 +50:05:56.9 -- not an asteroid (will add it to exclusion list)
00:14:41.96 +46:51:20.8 -- not an asteroid (will add it to exclusion list)
23:37:21.30 +46:30:57.3 -- not an asteroid (will add it to exclusion list)
23:48:42.61 +46:14:34.8 -- not an asteroid (will add it to exclusion list)
23:58:41.26 +48:31:40.3 -- not an asteroid (will add it to exclusion list)
23:57:30.24 +48:17:26.3 -- not an asteroid (will add it to exclusion list)
23:50:51.89 +43:04:44.7 -- not an asteroid (will add it to exclusion list)
23:41:22.75 +46:52:23.8 -- not an asteroid (will add it to exclusion list)
00:07:52.40 +44:04:40.8 -- not an asteroid (will add it to exclusion list)
23:51:58.92 +49:01:24.8 -- not an asteroid (will add it to exclusion list)
23:40:11.01 +45:02:53.6 -- not an asteroid (will add it to exclusion list)
23:34:59.81 +46:03:42.4 -- not an asteroid (will add it to exclusion list)
00:06:03.42 +49:37:34.6 -- not an asteroid (will add it to exclusion list)
23:48:29.60 +46:16:21.9 -- not an asteroid (will add it to exclusion list)
23:42:09.57 +44:44:15.8 -- not an asteroid (will add it to exclusion list)
00:12:42.80 +44:18:43.0 -- not an asteroid (will add it to exclusion list)
00:10:16.89 +49:00:01.5 -- not an asteroid (will add it to exclusion list)
00:05:31.30 +48:29:22.4 -- not an asteroid (will add it to exclusion list)
00:15:45.59 +45:30:23.6 -- not an asteroid (will add it to exclusion list)
00:01:37.73 +44:41:34.4 -- not an asteroid (will add it to exclusion list)
23:50:37.84 +47:30:33.5 -- not an asteroid (will add it to exclusion list)
23:45:20.72 +44:17:43.0 -- not an asteroid (will add it to exclusion list)
23:43:30.36 +47:20:00.6 -- not an asteroid (will add it to exclusion list)
23:52:55.93 +48:28:15.9 -- not an asteroid (will add it to exclusion list)
23:35:37.75 +43:44:51.8 -- not an asteroid (will add it to exclusion list)
23:39:25.53 +45:44:14.1 -- not an asteroid (will add it to exclusion list)
00:16:05.85 +46:59:40.2 -- not an asteroid (will add it to exclusion list)
23:48:13.24 +47:05:59.1 -- not an asteroid (will add it to exclusion list)
23:55:59.49 +48:12:26.6 -- not an asteroid (will add it to exclusion list)
23:54:25.47 +48:54:43.0 -- not an asteroid (will add it to exclusion list)
23:44:56.16 +50:07:12.0 -- not an asteroid (will add it to exclusion list)
00:02:09.82 +42:08:07.2 -- not an asteroid (will add it to exclusion list)
00:10:38.93 +48:37:01.3 -- not an asteroid (will add it to exclusion list)
23:40:11.38 +48:47:40.4 -- not an asteroid (will add it to exclusion list)
23:57:14.32 +45:56:53.5 -- not an asteroid (will add it to exclusion list)
00:18:30.42 +43:59:38.6 -- not an asteroid (will add it to exclusion list)
00:05:48.54 +45:47:23.2 -- not an asteroid (will add it to exclusion list)
23:43:31.91 +47:19:18.6 -- not an asteroid (will add it to exclusion list)
23:43:03.30 +49:07:40.0 -- not an asteroid (will add it to exclusion list)
00:09:56.46 +46:22:42.7 -- not an asteroid (will add it to exclusion list)
00:01:42.40 +46:36:22.1 -- not an asteroid (will add it to exclusion list)
23:57:42.49 +48:23:29.1 -- not an asteroid (will add it to exclusion list)
00:01:31.96 +47:56:37.5 -- not an asteroid (will add it to exclusion list)
23:43:18.08 +43:21:01.5 -- not an asteroid (will add it to exclusion list)
23:58:57.37 +44:34:56.5 -- not an asteroid (will add it to exclusion list)
23:46:58.69 +48:49:35.7 -- not an asteroid (will add it to exclusion list)
00:10:08.09 +50:09:19.5 -- not an asteroid (will add it to exclusion list)
23:58:27.09 +48:35:38.7 -- not an asteroid (will add it to exclusion list)
23:45:46.47 +48:26:37.5 -- not an asteroid (will add it to exclusion list)
00:01:22.58 +46:44:47.0 -- not an asteroid (will add it to exclusion list)
23:38:09.87 +46:10:52.9 -- not an asteroid (will add it to exclusion list)
23:45:02.59 +44:47:30.5 -- not an asteroid (will add it to exclusion list)
23:54:39.78 +49:17:01.7 -- not an asteroid (will add it to exclusion list)
23:46:42.47 +44:27:24.3 -- not an asteroid (will add it to exclusion list)
00:21:48.81 +44:52:17.8 -- not an asteroid (will add it to exclusion list)
00:19:50.27 +47:42:36.6 -- not an asteroid (will add it to exclusion list)
23:50:36.09 +47:31:26.5 -- not an asteroid (will add it to exclusion list)
23:54:35.04 +43:11:16.7 -- not an asteroid (will add it to exclusion list)
23:34:07.49 +46:20:03.2 -- not an asteroid (will add it to exclusion list)
23:39:51.84 +47:45:01.3 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
00:01:22.58 +46:44:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:01:31.96 +47:56:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:01:37.73 +44:41:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:01:42.40 +46:36:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:02:09.82 +42:08:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:03:07.80 +50:05:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:05:31.30 +48:29:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:05:48.54 +45:47:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:06:03.42 +49:37:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:07:52.40 +44:04:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:09:56.46 +46:22:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:10:08.09 +50:09:19.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:10:16.89 +49:00:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:10:38.93 +48:37:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:10:55.01 +48:15:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:12:42.80 +44:18:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:14:41.96 +46:51:20.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:15:45.59 +45:30:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:16:05.85 +46:59:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:18:30.42 +43:59:38.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:19:50.27 +47:42:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:21:48.81 +44:52:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:22:05.07 +44:08:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:34:07.49 +46:20:03.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:34:59.81 +46:03:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:35:37.75 +43:44:51.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:36:39.60 +42:43:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:37:21.30 +46:30:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:37:29.46 +49:59:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:38:09.87 +46:10:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:39:25.53 +45:44:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:39:51.84 +47:45:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:40:11.01 +45:02:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:40:11.38 +48:47:40.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:41:22.75 +46:52:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:42:09.57 +44:44:15.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:43:03.30 +49:07:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:43:18.08 +43:21:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:43:30.36 +47:20:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:43:31.91 +47:19:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:43:33.28 +50:00:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:44:56.16 +50:07:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:45:02.30 +43:55:29.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:45:02.59 +44:47:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:45:20.72 +44:17:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:45:46.47 +48:26:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:46:42.47 +44:27:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:46:58.69 +48:49:35.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:48:13.24 +47:05:59.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:48:29.60 +46:16:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:48:42.61 +46:14:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:50:36.09 +47:31:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:50:37.84 +47:30:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:50:51.89 +43:04:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:51:51.58 +48:26:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:51:58.92 +49:01:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:52:55.93 +48:28:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:54:25.47 +48:54:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:54:35.04 +43:11:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:54:39.78 +49:17:01.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:55:59.49 +48:12:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:57:14.32 +45:56:53.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:57:30.24 +48:17:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:57:42.49 +48:23:29.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:27.09 +48:35:38.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:41.26 +48:31:40.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:57.37 +44:34:56.5 -- 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)
00:01:22.58 +46:44:47.0 -- not a known variable star
00:01:31.96 +47:56:37.5 -- not a known variable star
00:01:37.73 +44:41:34.4 -- not a known variable star
00:01:42.40 +46:36:22.1 -- not a known variable star
00:02:09.82 +42:08:07.2 -- not a known variable star
00:03:07.80 +50:05:56.9 -- not a known variable star
00:05:31.30 +48:29:22.4 -- not a known variable star
00:05:48.54 +45:47:23.2 -- not a known variable star
00:06:03.42 +49:37:34.6 -- not a known variable star
00:07:52.40 +44:04:40.8 -- not a known variable star
00:09:56.46 +46:22:42.7 -- not a known variable star
00:10:08.09 +50:09:19.5 -- not a known variable star
00:10:16.89 +49:00:01.5 -- a known variable star
00:10:38.93 +48:37:01.3 -- not a known variable star
00:10:55.01 +48:15:31.7 -- a known variable star
00:12:42.80 +44:18:43.0 -- not a known variable star
00:14:41.96 +46:51:20.8 -- not a known variable star
00:15:45.59 +45:30:23.6 -- not a known variable star
00:16:05.85 +46:59:40.2 -- not a known variable star
00:18:30.42 +43:59:38.6 -- not a known variable star
00:19:50.27 +47:42:36.6 -- a known variable star
00:21:48.81 +44:52:17.8 -- a known variable star
00:22:05.07 +44:08:44.0 -- a known variable star
23:34:07.49 +46:20:03.2 -- a known variable star
23:34:59.81 +46:03:42.4 -- not a known variable star
23:35:37.75 +43:44:51.8 -- not a known variable star
23:36:39.60 +42:43:33.5 -- not a known variable star
23:37:21.30 +46:30:57.3 -- not a known variable star
23:37:29.46 +49:59:56.1 -- not a known variable star
23:38:09.87 +46:10:52.9 -- not a known variable star
23:39:25.53 +45:44:14.1 -- not a known variable star
23:39:51.84 +47:45:01.3 -- a known variable star
23:40:11.01 +45:02:53.6 -- not a known variable star
23:40:11.38 +48:47:40.4 -- a known variable star
23:41:22.75 +46:52:23.8 -- not a known variable star
23:42:09.57 +44:44:15.8 -- not a known variable star
23:43:03.30 +49:07:40.0 -- not a known variable star
23:43:18.08 +43:21:01.5 -- not a known variable star
23:43:30.36 +47:20:00.6 -- not a known variable star
23:43:31.91 +47:19:18.6 -- not a known variable star
23:43:33.28 +50:00:45.0 -- not a known variable star
23:44:56.16 +50:07:12.0 -- not a known variable star
23:45:02.30 +43:55:29.4 -- a known variable star
23:45:02.59 +44:47:30.5 -- not a known variable star
23:45:20.72 +44:17:43.0 -- not a known variable star
23:45:46.47 +48:26:37.5 -- a known variable star
23:46:42.47 +44:27:24.3 -- not a known variable star
23:46:58.69 +48:49:35.7 -- a known variable star
23:48:13.24 +47:05:59.1 -- not a known variable star
23:48:29.60 +46:16:21.9 -- not a known variable star
23:48:42.61 +46:14:34.8 -- not a known variable star
23:50:36.09 +47:31:26.5 -- not a known variable star
23:50:37.84 +47:30:33.5 -- not a known variable star
23:50:51.89 +43:04:44.7 -- a known variable star
23:51:51.58 +48:26:38.5 -- not a known variable star
23:51:58.92 +49:01:24.8 -- not a known variable star
23:52:55.93 +48:28:15.9 -- not a known variable star
23:54:25.47 +48:54:43.0 -- not a known variable star
23:54:35.04 +43:11:16.7 -- a known variable star
23:54:39.78 +49:17:01.7 -- a known variable star
23:55:59.49 +48:12:26.6 -- not a known variable star
23:57:14.32 +45:56:53.5 -- not a known variable star
23:57:30.24 +48:17:26.3 -- a known variable star
23:57:42.49 +48:23:29.1 -- not a known variable star
23:58:27.09 +48:35:38.7 -- not a known variable star
23:58:41.26 +48:31:40.3 -- not a known variable star
23:58:57.37 +44:34:56.5 -- not a known variable star
Found 52 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
67 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 67 (excluding asteroids and hot pixels, 52 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)2461136.97768021 -observatory V36
23:21:37.61 -06:19:52.0 Mercury (0.3mag)
02:22:51.12 +13:58:30.5 Venus (-3.9mag)
23:50:43.46 -02:07:15.1 Mars (1.2mag)
07:08:48.14 +22:52:17.0 Jupiter (-2.2mag)
00:24:53.50 +00:22:02.4 Saturn (0.9mag)
03:45:46.64 +19:41:16.1 Uranus (5.8mag)
00:09:34.13 -00:23:25.6 Neptune (7.8mag)
20:33:15.25 -22:52:29.1 Pluto (14.5mag)
16:09:26.66 -27:03:44.3 Moon (-11.4mag)
-rw-r--r-- 1 apache apache 362 Apr 6 07:15 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461136.97768021:
07:08:44.29 +22:52:21.9 Io (5.7mag)
07:08:58.41 +22:51:54.0 Europa (5.8mag)
07:08:47.58 +22:52:25.5 Ganymede (5.3mag)
07:08:16.54 +22:53:13.1 Callisto (6.5mag)
07:12:30.56 +22:44:38.1 Himalia (15.3mag)
07:08:52.28 +22:52:07.6 Thebe (16.2mag)
07:12:28.66 +23:13:27.9 Elara (17.2mag)
07:07:02.16 +23:37:16.4 Pasiphae (17.3mag)
07:17:19.65 +22:49:15.2 Carme (18.4mag)
00:24:49.15 +00:22:01.7 Titan (8.8mag)
00:24:50.16 +00:22:14.2 Rhea (10.1mag)
00:24:53.41 +00:23:34.0 Iapetus (11.5mag)
00:24:56.29 +00:21:50.0 Hyperion (14.8mag)
00:26:37.52 +00:31:49.8 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 6 07:15 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461136.97768021:
14:47:38.25 -08:35:25.7 JWST
17:20:33.77 +41:51:28.2 Chandra
09:09:31.85 -52:17:16.9 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 6 07:15 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461136.97768021 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:47:17.48 -28:15:02.9 13.9mag P/2010 H2 (Vales)
05:00:16.15 -70:07:58.8 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:30:37.04 +31:22:39.0 17.1mag C/2017 K2 (PANSTARRS)
17:30:56.59 +09:24:17.5 17.6mag C/2021 G2 (ATLAS)
23:07:26.68 +28:52:40.2 17.0mag C/2022 E2 (ATLAS)
04:18:18.99 +25:46:20.5 15.9mag C/2022 N2 (PANSTARRS)
09:01:53.62 +31:54:40.2 16.1mag C/2022 QE78 (ATLAS)
08:30:00.31 -01:11:59.9 17.3mag C/2022 R6 (PANSTARRS)
18:55:32.91 +17:43:11.0 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:43:26.24 -11:39:24.1 17.6mag P/2023 B1 (PANSTARRS)
09:12:39.86 -13:27:16.1 17.5mag C/2023 F3 (ATLAS)
21:43:49.04 +62:23:09.9 17.5mag C/2023 H5 (Lemmon)
19:26:14.20 -03:36:40.4 14.3mag C/2023 R1 (PANSTARRS)
21:42:34.57 +84:38:49.9 17.8mag C/2023 X2 (Lemmon)
06:14:35.53 +63:34:49.5 17.0mag C/2024 A1 (ATLAS)
04:51:45.46 +14:40:51.9 10.4mag C/2024 E1 (Wierzchos)
16:24:56.78 +04:49:29.4 17.4mag C/2024 G6 (ATLAS)
20:17:39.54 +12:45:25.2 14.7mag C/2024 J3 (ATLAS)
03:18:00.77 -23:52:36.1 16.4mag C/2024 T5 (ATLAS)
05:08:55.83 +47:45:24.1 17.7mag C/2025 J1 (Borisov)
14:17:57.34 +37:40:43.2 14.8mag C/2025 L1 (ATLAS)
03:10:47.37 -24:47:22.7 17.8mag C/2025 Q3 (ATLAS)
22:54:20.03 +19:50:16.2 10.1mag C/2025 R3 (PANSTARRS)
12:58:15.91 +02:24:39.2 17.5mag C/2025 Y1 (ATLAS)
01:36:15.12 +04:35:25.9 7.6mag C/2026 A1 (MAPS)
23:31:40.80 +35:18:26.8 14.3mag C/2026 B2 (Sun-Gao)
18:24:20.79 -10:12:18.6 12.4mag 10P/Tempel
15:12:32.95 +04:05:21.4 13.2mag 24P/Schaumasse
11:05:40.38 -01:51:12.1 15.7mag 29P/Schwassmann-Wachmann
17:56:55.31 -09:58:53.7 17.7mag 40P/Vaisala
10:38:48.87 -04:55:16.8 16.7mag 43P/Wolf-Harrington
01:33:59.68 +15:50:45.8 17.1mag 47P/Ashbrook-Jackson
06:53:49.22 +39:01:14.8 17.0mag 63P/Wild
23:16:41.40 -12:37:09.3 15.7mag 65P/Gunn
03:38:24.53 +17:50:40.8 15.8mag 76P/West-Kohoutek-Ikemura
00:44:42.25 +06:20:32.3 14.4mag 78P/Gehrels
22:33:27.81 -12:11:19.4 14.5mag 88P/Howell
01:43:57.24 +18:01:42.1 15.1mag 93P/Lovas
04:37:25.91 +31:44:43.2 16.3mag 123P/West-Hartley
08:18:11.91 +42:45:26.4 16.2mag 124P/Mrkos
02:18:39.18 +13:17:24.0 16.4mag 128P/Shoemaker-Holt
02:28:57.42 +13:17:28.1 17.5mag 131P/Mueller
00:37:18.77 +09:43:19.0 11.2mag 141P/Machholz
00:47:16.03 +01:18:21.5 11.3mag 141P-A/Machholz
23:37:40.02 -02:20:00.6 14.0mag 141P-D/Machholz
01:16:26.12 +02:58:31.5 17.9mag 141P-I/Machholz
00:35:56.03 -06:16:36.5 15.2mag 162P/SidingSpring
10:30:52.81 +31:29:20.3 17.8mag 164P/Christensen
06:18:57.32 +24:30:57.7 17.8mag 198P/ODAS
15:08:12.03 -01:09:34.8 17.4mag 210P/Christensen
21:09:50.32 -13:45:10.5 17.4mag 218P/LINEAR
17:12:45.52 -15:02:29.9 16.2mag 235P/LINEAR
05:14:15.53 +33:52:59.6 16.6mag 240P/NEAT
07:34:18.58 -06:15:09.1 17.6mag 242P/Spahr
15:45:51.40 +06:19:48.1 17.5mag 391P/Kowalski
07:30:59.92 +21:18:49.6 17.6mag 450P/LONEOS
05:22:18.90 +45:35:37.9 17.4mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 6 07:15 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
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
11:19:50.70 -27:51:49.80 SN2026gvk 2026-03-30 15.48
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
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
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
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
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
13:06:01.89 -15:50:13.40 AT2026fdy 2026-03-10.5 16.39
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
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
09:27:45.33 -37:49:33.00 ASASSN-26bk 2026-03-2.06 13.58
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
18:03:39.29 +19:58:46.30 ASASSN-26be 2026-02-25.56 14.95
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
11:50:37.32 +55:21:13.70 SN 2026dix 2026-02-21.43 16.39
16:21:19.69 -63:47:29.40 ASASSN-26az 2026-02-21.03 17.02
02:45:30.93 -54:17:43.10 SN 2026cju 2026-02-21.04 17.54
01:58:40.68 +47:34:50.10 ASASSN-26av 2026-02-21.09 15.97
18:35:53.01 -42:31:38.90 ASASSN-26aw 2026-02-21.12 15.89
11:40:18.88 -39:45:09.20 ASASSN-26ax 2026-02-21.08 15.73
02:26:23.52 -51:42:29.80 ASASSN-26ay 2026-02-21.04 13.93
08:46:07.66 +01:17:43.90 ASASSN-26ba 2026-02-20.23 15.43
14:15:47.69 -48:05:16.40 SN2026dez 2026-02-19.19 15.93
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.22 -11:25:16.10 AT2026bzh 2026-02-12.16 17.22
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
06:26:33.34 -54:06:39.90 AT2026cih 2026-02-8.06 17.26
23:08:59.40 -88:59:11.60 SN 2026bsu 2026-02-8.03 16.02
01:04:14.94 -62:31:02.30 SN 2026azk 2026-02-8.04 16.41
-rw-r--r-- 1 apache apache 5.8K Apr 6 07:15 asassn_transients_list.txt
############################################################
Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
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
-rw-r--r-- 1 apache apache 187K Apr 6 07:15 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
03:28:17.606 -27:41:55.66 AT 2026huw 2026-03-22.00 22.983
03:33:45.089 -26:56:57.92 AT 2026huv 2026-03-22.00 22.754
03:34:56.740 -28:52:22.60 AT 2026huu 2026-03-07.04 22.581
09:54:07.147 +02:31:26.93 AT 2026hut 2026-02-23.17 21.969
09:58:55.929 +02:50:43.70 AT 2026hus 2026-03-07.13 23.075
18:10:28.390 -00:15:37.94 AT 2026hur 2026-03-29.85 15.81
12:25:24.050 -04:47:33.90 AT 2026huq 2026-03-29.26 17.856
20:57:23.355 -24:44:41.72 AT 2026hup 2026-03-29.38 18.333
15:25:55.004 +07:49:25.15 AT 2026huo 2026-03-29.08 19.198
16:37:31.883 -66:34:41.26 AT 2026hun 2026-03-19.31 19.546
04:02:43.436 -46:55:47.58 AT 2026hum 2026-02-19.05 22.54
06:43:09.512 +11:30:54.69 AT 2026hul 2026-03-29.21 19.022
14:19:10.599 -33:29:33.62 AT 2026huk 2026-03-29.24 19.7
13:34:24.360 +36:48:31.82 AT 2026huj 2026-03-20.71 20.85
07:36:21.380 +15:56:54.55 AT 2026hui 2026-03-18.71 20.7
11:53:11.050 +21:20:34.15 AT 2026huh 2026-03-17.78 21.68
11:11:02.080 +21:51:43.20 AT 2026hug 2026-03-17.78 21.19
11:58:25.850 +16:51:27.33 AT 2026huf 2026-03-17.78 21.62
07:42:32.090 +18:28:41.88 AT 2026hue 2026-03-17.76 21.39
09:40:01.520 +16:17:02.86 AT 2026hud 2026-03-17.76 20.71
-rw-r--r-- 1 apache apache 30K Apr 6 07:15 tns_transients_list.txt
