This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF
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 09.4724* 00 12 06.68 +48 12 20.2 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J001206.75+481222.5,2461139.9724,10.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J001206.75+481222.5 20260409.4724 10.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 23 45 02.52 +43 55 27.3 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
EY And,2461139.9724,10.44,0.05,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
EY And 20260409.4724 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 09.4724* 23 50 51.95 +43 04 44.2 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
EZ And,2461139.9724,11.19,0.05,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
EZ And 20260409.4724 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 09.4724* 00 22 05.02 +44 08 44.1 10.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 3656996,2461139.9724,10.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 3656996 20260409.4724 10.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 23 55 55.14 +49 31 44.9 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.9724,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.4724 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 23 44 27.05 +49 42 04.2 12.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J356.1125+49.6989,2461139.9724,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J356.1125+49.6989 20260409.4724 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 23 51 51.55 +48 26 39.8 12.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J357.9705+48.4419,2461139.9724,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J357.9705+48.4419 20260409.4724 12.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 23 37 29.56 +49 59 54.6 12.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1943698346142347136,2461139.9724,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1943698346142347136 20260409.4724 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 23 43 33.14 +50 00 46.1 12.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1943568466332031104,2461139.9724,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1943568466332031104 20260409.4724 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 23 48 52.09 +42 06 29.8 11.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1922492890007272448,2461139.9724,11.68,0.05,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 1922492890007272448 20260409.4724 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 09.4724* 00 03 05.30 +49 49 28.5 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 393891523740267136,2461139.9724,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 393891523740267136 20260409.4724 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 00 14 41.90 +46 51 20.2 11.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 392207548658221312,2461139.9724,11.07,0.05,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 392207548658221312 20260409.4724 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 09.4724* 23 48 42.64 +46 14 34.6 10.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1927283771411171200,2461139.9724,10.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1927283771411171200 20260409.4724 10.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 23 38 24.83 +47 25 52.6 10.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1940031681020915072,2461139.9724,10.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1940031681020915072 20260409.4724 10.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 23 57 30.24 +48 17 25.2 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1939610705511944064,2461139.9724,9.46,0.05,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 20260409.4724 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 09.4724* 23 41 22.67 +46 52 23.6 10.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1939240926002369536,2461139.9724,10.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1939240926002369536 20260409.4724 10.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 23 51 58.95 +49 01 25.7 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1940551268987081856,2461139.9724,10.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1940551268987081856 20260409.4724 10.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 23 46 23.33 +49 27 14.6 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1940470695399543424,2461139.9724,10.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1940470695399543424 20260409.4724 10.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 23 48 29.60 +46 16 21.7 10.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1927284797904773120,2461139.9724,10.87,0.05,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 1927284797904773120 20260409.4724 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 09.4724* 23 40 10.87 +45 02 53.2 10.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1926756143267842048,2461139.9724,10.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1926756143267842048 20260409.4724 10.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 00 06 03.38 +49 37 35.0 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 393829190871939328,2461139.9724,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 393829190871939328 20260409.4724 10.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 23 42 09.53 +44 44 16.1 11.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1926630524064281088,2461139.9724,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1926630524064281088 20260409.4724 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 23 56 39.19 +48 26 57.1 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1939607716215581440,2461139.9724,11.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1939607716215581440 20260409.4724 11.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 23 50 37.81 +47 30 33.0 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J357.6529+47.5164,2461139.9724,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J357.6529+47.5164 20260409.4724 11.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 23 47 35.34 +49 58 04.0 11.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1943873924406057984,2461139.9724,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1943873924406057984 20260409.4724 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 00 10 16.82 +49 00 01.6 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 393561876404915840,2461139.9724,11.07,0.05,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 20260409.4724 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 09.4724* 00 15 45.53 +45 30 22.8 11.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.9724,10.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.4724 10.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 00 05 31.31 +48 29 22.5 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 393374787630869888,2461139.9724,11.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 393374787630869888 20260409.4724 11.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 23 45 20.74 +44 17 42.8 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.9724,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.4724 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 00 02 09.77 +42 08 06.7 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.9724,11.19,0.05,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 20260409.4724 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 09.4724* 00 16 05.80 +46 59 38.2 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.9724,11.30,0.05,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
target 20260409.4724 11.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 23 39 25.64 +45 44 14.3 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.9724,11.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.4724 11.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 23 48 13.17 +47 05 59.5 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J357.0571+47.0984,2461139.9724,11.46,0.05,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
ATO J357.0571+47.0984 20260409.4724 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 23 54 25.40 +48 54 44.4 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J358.5960+48.9077,2461139.9724,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J358.5960+48.9077 20260409.4724 11.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 00 24 01.80 +44 14 42.1 11.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 varaible 382758654967939840,2461139.9724,11.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 varaible 382758654967939840 20260409.4724 11.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 00 24 07.63 +46 17 09.1 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 391990639928120576,2461139.9724,11.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 391990639928120576 20260409.4724 11.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 00 01 42.34 +46 36 22.7 11.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J000.4293+46.6268,2461139.9724,11.52,0.05,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
ATO J000.4293+46.6268 20260409.4724 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 09.4724* 23 43 17.92 +43 21 01.1 11.6 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.9724,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.4724 11.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 23 40 11.23 +48 47 39.8 11.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1940343186409018112,2461139.9724,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1940343186409018112 20260409.4724 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 00 17 32.51 +50 15 57.9 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.9724,11.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.4724 11.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 00 18 30.34 +43 59 38.6 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J004.6157+43.9987,2461139.9724,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J004.6157+43.9987 20260409.4724 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 00 17 36.21 +50 17 52.5 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.9724,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.4724 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 00 09 56.38 +46 22 43.5 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.9724,11.52,0.05,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
target 20260409.4724 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 09.4724* 23 52 22.08 +48 28 25.5 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J358.0980+48.4799,2461139.9724,11.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J358.0980+48.4799 20260409.4724 11.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 00 05 48.56 +45 47 22.6 11.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.9724,11.44,0.05,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 20260409.4724 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 09.4724* 23 36 51.82 +43 17 16.3 11.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.9724,11.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.4724 11.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 23 43 31.98 +47 19 19.4 11.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.9724,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.4724 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 23 46 58.79 +48 49 35.9 11.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1940577897784457856,2461139.9724,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1940577897784457856 20260409.4724 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 23 55 37.90 +48 37 56.0 11.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.9724,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.4724 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 23 34 39.48 +48 12 03.6 12.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.9724,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.4724 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 23 45 05.07 +49 44 13.1 12.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J356.2628+49.7436,2461139.9724,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J356.2628+49.7436 20260409.4724 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 23 40 08.70 +49 47 06.9 12.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1943726658567506304,2461139.9724,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1943726658567506304 20260409.4724 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 23 50 07.59 +47 35 53.9 11.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J357.5345+47.5961,2461139.9724,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J357.5345+47.5961 20260409.4724 11.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 23 48 38.73 +43 37 24.9 11.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1925857739185928320,2461139.9724,11.74,0.05,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
Gaia DR3 1925857739185928320 20260409.4724 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 09.4724* 00 04 42.68 +47 25 08.1 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 387230579213845504,2461139.9724,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 387230579213845504 20260409.4724 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 23 41 54.48 +49 26 18.6 12.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J355.4758+49.4271,2461139.9724,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J355.4758+49.4271 20260409.4724 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 23 54 01.90 +44 33 36.0 11.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.9724,11.79,0.05,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 20260409.4724 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 09.4724* 23 43 26.66 +47 19 49.1 12.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.9724,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.4724 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 23 43 18.75 +43 20 17.7 11.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.9724,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.4724 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 00 01 32.01 +47 56 38.0 11.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.9724,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.4724 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 23 42 58.04 +47 13 12.6 12.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J355.7232+47.2222,2461139.9724,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J355.7232+47.2222 20260409.4724 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 00 10 11.74 +47 19 03.0 11.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.9724,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.4724 11.91CV 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 09.4724* 23 48 35.97 +46 15 51.3 12.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.9724,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.4724 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 00 01 22.46 +46 44 46.4 11.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.9724,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.4724 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 00 06 30.39 +47 25 01.3 11.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 393033492346401536,2461139.9724,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 393033492346401536 20260409.4724 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 23 57 20.51 +48 06 20.6 12.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J359.3365+48.1062,2461139.9724,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J359.3365+48.1062 20260409.4724 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 23 54 57.59 +46 52 39.2 12.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.9724,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.4724 12.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 23 37 54.57 +43 22 54.4 12.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J354.4777+43.3809,2461139.9724,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J354.4777+43.3809 20260409.4724 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 00 08 25.19 +44 57 38.4 11.8 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.9724,11.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.4724 11.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 00 05 50.14 +49 36 52.2 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.9724,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.4724 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 00 02 17.32 +44 32 06.8 11.9 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.9724,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.4724 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 00 03 11.41 +45 52 59.3 12.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.9724,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.4724 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 23 35 06.08 +47 31 15.9 12.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.9724,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.4724 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 00 02 46.17 +47 14 34.9 12.0 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.9724,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.4724 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 00 05 30.40 +46 40 47.2 12.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.9724,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.4724 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 23 51 40.59 +50 05 54.1 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.9724,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.4724 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 23 53 47.74 +50 06 37.2 12.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.9724,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.4724 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 23 44 49.93 +44 01 25.8 12.2 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J356.2109+44.0114,2461139.9724,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J356.2109+44.0114 20260409.4724 12.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 23 35 22.79 +45 57 50.1 12.5 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1937585710028510464,2461139.9724,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1937585710028510464 20260409.4724 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 00 19 50.11 +47 42 37.4 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0960 Cas,2461139.9724,11.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0960 Cas 20260409.4724 11.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 00 21 48.80 +44 52 18.4 10.7 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0021489+445219,2461139.9724,10.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0021489+445219 20260409.4724 10.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 00 10 54.95 +48 15 31.7 9.4 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
LD 323,2461139.9724,9.38,0.05,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
LD 323 20260409.4724 9.38CV 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 09.4724* 23 50 36.04 +47 31 26.4 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J357.6529+47.5164,2461139.9724,10.44,0.05,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 20260409.4724 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 09.4724* 23 34 07.44 +46 20 02.8 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0339 And,2461139.9724,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0339 And 20260409.4724 11.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.4724* 23 54 35.04 +43 11 17.0 10.3 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2354350+431115,2461139.9724,10.31,0.05,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
NSVS J2354350+431115 20260409.4724 10.31CV 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 09.4724* 23 39 51.85 +47 45 01.7 11.1 U And 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
EX And,2461139.9724,11.07,0.05,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
EX And 20260409.4724 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
## 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: 2461139.97272052 09.04.2026 11:20:33.053 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.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: 4 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): 17711
Objects passed selection criteria: 17629
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: 11950.8
Average stars matched: 11049 (92.4544 %)
Memory usage VmPeak: 121820 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 9 06:22:37 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: 2461139.97272052 09.04.2026 11:20:33.053 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 132
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: 28 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): 115655
Objects passed selection criteria: 115329
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 82628.5
Average stars matched: 75358.5 (91.2016 %)
Memory usage VmPeak: 2662616 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 9 06:25:04 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_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.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_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.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: 2461139.97214101
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits exists and is non-empty
Saving wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits to local_wcs_cache/
'wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits' -> 'local_wcs_cache/wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits'
wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits exists and is non-empty
Saving wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits to local_wcs_cache/
'wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits' -> 'local_wcs_cache/wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits'
wcs_fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits exists and is non-empty
Saving wcs_fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits to local_wcs_cache/
'wcs_fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits' -> 'local_wcs_cache/wcs_fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits'
wcs_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.fits exists and is non-empty
Saving wcs_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.fits to local_wcs_cache/
'wcs_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.fits' -> 'local_wcs_cache/wcs_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.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 00:00:03.995 +46:01:54.33
Angular distance between the image centers 0.0772 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 00:00:07.069 +46:01:49.67
Angular distance between the image centers 0.0713 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 00:00:03.995 +46:01:54.33
Second-epoch second image center 00:00:07.069 +46:01:49.67
Angular distance between the image centers 0.00899 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.IcBxBrnDOG
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.sfAeHC6P2D
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_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits &> /tmp/tmp.LQYF1WDDiU
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.fits &> /tmp/tmp.OXeVqXIL0w
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.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_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits
2.5 pix fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.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
13.9 mag. fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits
13.8 mag. fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 11.1 (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.IcBxBrnDOG (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_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits 567.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits' -> 'wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
WCS_IMAGE_NAME=wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
WCS-calibrated image found: wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
Checking if the catalog wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits.cat corresponding to the image wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits alredy exist and is non-empty...
Catalog wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits.cat corresponding to the image wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
WCS catalog name: wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2256, passed=21978
Got 21978 stars (including 19693 good ones) from the SExtractor catalog wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits.cat
util/solve_plate_with_UCAC5 got 21978 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 924.9'
Seting catalog search parameters based on the expected field of view 924.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012846 (46.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010277 (37.0 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 348.4507 through 0 to 12.6948, gap 12.6948 to 348.4507
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 40.0 to 51.2)
Done reading UCAC5 zone files...
Matched 203 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 146 matched stars entering correct_measured_positions(), 68 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 10.79"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 141 matched stars entering correct_measured_positions(), 2320 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 11.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 348.4573 through 0 to 12.6998, gap 12.6998 to 348.4573
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 40.0 to 51.2)
Done reading UCAC5 zone files...
Matched 230 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 175 matched stars entering correct_measured_positions(), 2338 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 11.32"
Accuracy estimation diagnostic: 173 matched stars entering correct_measured_positions(), 3009 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.42"
Excluding outliers - 173 stars left (next iteration limit 155)
The image catalog is written to wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits -region wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.sfAeHC6P2D (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_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits 567.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits' -> 'wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
WCS_IMAGE_NAME=wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
WCS-calibrated image found: wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
Checking if the catalog wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits.cat corresponding to the image wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits alredy exist and is non-empty...
Catalog wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits.cat corresponding to the image wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
WCS catalog name: wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2250, passed=22050
Got 22050 stars (including 19777 good ones) from the SExtractor catalog wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits.cat
util/solve_plate_with_UCAC5 got 22050 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 924.9'
Seting catalog search parameters based on the expected field of view 924.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012846 (46.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010277 (37.0 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 348.4512 through 0 to 12.6947, gap 12.6947 to 348.4512
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 40.0 to 51.2)
Done reading UCAC5 zone files...
Matched 202 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 142 matched stars entering correct_measured_positions(), 69 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 11.99"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 135 matched stars entering correct_measured_positions(), 2248 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 12.05"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 348.4583 through 0 to 12.7006, gap 12.7006 to 348.4583
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 40.0 to 51.2)
Done reading UCAC5 zone files...
Matched 223 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 175 matched stars entering correct_measured_positions(), 2273 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 12.04"
Accuracy estimation diagnostic: 172 matched stars entering correct_measured_positions(), 3100 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 10.65"
Excluding outliers - 172 stars left (next iteration limit 148)
The image catalog is written to wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits -region wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.LQYF1WDDiU (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_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.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_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits
WCS_IMAGE_NAME=wcs_fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits
WCS-calibrated image found: wcs_fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits
Checking if the catalog wcs_fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits.cat corresponding to the image wcs_fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits alredy exist and is non-empty...
Catalog wcs_fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits.cat corresponding to the image wcs_fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.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_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits
WCS catalog name: wcs_fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=638, passed=9412
Got 9412 stars (including 8771 good ones) from the SExtractor catalog wcs_fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits.cat
util/solve_plate_with_UCAC5 got 9412 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010430 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 347.5551 through 0 to 12.1371, gap 12.1371 to 347.5551
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.2 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...
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 912 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.78"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 9171 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
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 347.5544 through 0 to 12.1375, gap 12.1375 to 347.5544
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.2 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
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 9172 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 9172 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.82"
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_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits -region wcs_fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.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.OXeVqXIL0w (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_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.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_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.fits
WCS_IMAGE_NAME=wcs_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.fits
WCS-calibrated image found: wcs_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.fits
Checking if the catalog wcs_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.fits.cat corresponding to the image wcs_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.fits alredy exist and is non-empty...
Catalog wcs_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.fits.cat corresponding to the image wcs_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.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_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.fits
WCS catalog name: wcs_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=573, passed=9072
Got 9072 stars (including 8490 good ones) from the SExtractor catalog wcs_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.fits.cat
util/solve_plate_with_UCAC5 got 9072 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010430 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 347.5550 through 0 to 12.1363, gap 12.1363 to 347.5550
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.2 to 51.3)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 907 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 8859 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.74"
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 347.5544 through 0 to 12.1367, gap 12.1367 to 347.5544
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.2 to 51.3)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 8861 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.74"
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 8861 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.80"
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_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.fits -region wcs_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.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_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/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_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/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_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/wcs_fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits'
Saving fully-calibrated image wcs_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/wcs_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.fits'
Preparing the HTML report for the field And-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out15590.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31926.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31938.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32998.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 43s
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: 3s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31926_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 31926_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31938_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 31938_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32998_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 32998_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15590_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 15590_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 46s
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 ####
00:22:05.02 +44:08:44.1
00:12:06.68 +48:12:20.2
23:45:02.52 +43:55:27.3
23:50:51.95 +43:04:44.2
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_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.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_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.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_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits
Creating symlink local_wcs_cache/wcs_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.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_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits exists and is non-empty
wcs_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.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 00:00:03.995 +46:01:54.33
Angular distance between the image centers 0.0772 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 00:00:07.069 +46:01:49.67
Angular distance between the image centers 0.0713 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 00:00:03.995 +46:01:54.33
Second-epoch second image center 00:00:07.069 +46:01:49.67
Angular distance between the image centers 0.00899 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.9Lyeuy83IB
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.ugzGNHx6WC
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_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits &> /tmp/tmp.fJXwFIQv76
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.fits &> /tmp/tmp.8kT6W7O0AI
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.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 107 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
2.4 pix fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits
2.3 pix fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.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
12.6 mag. fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits
12.6 mag. fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.fits
All-image limiting magnitude estimate: 12.6 (SNR ) 12.1 (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.9Lyeuy83IB (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_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits 567.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits' -> 'wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
WCS_IMAGE_NAME=wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
WCS-calibrated image found: wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
Checking if the catalog wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits.cat corresponding to the image wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits alredy exist and is non-empty...
Catalog wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits.cat corresponding to the image wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits
WCS catalog name: wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=47, blended=18012, passed=141962
Got 141962 stars (including 123722 good ones) from the SExtractor catalog wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits.cat
util/solve_plate_with_UCAC5 got 141962 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 924.9'
Seting catalog search parameters based on the expected field of view 924.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012846 (46.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010277 (37.0 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 348.4418 through 0 to 12.7147, gap 12.7147 to 348.4418
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.2)
Done reading UCAC5 zone files...
Matched 204 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 151 matched stars entering correct_measured_positions(), 79 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 10.98"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 145 matched stars entering correct_measured_positions(), 15623 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 12.14"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 348.4528 through 0 to 12.7273, gap 12.7273 to 348.4528
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.2)
Done reading UCAC5 zone files...
Matched 220 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 178 matched stars entering correct_measured_positions(), 15632 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 12.13"
Accuracy estimation diagnostic: 177 matched stars entering correct_measured_positions(), 18852 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 10.12"
Excluding outliers - 177 stars left (next iteration limit 159)
The image catalog is written to wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits -region wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_And-01-Q2b1x1_2025-12-26_19-50-42_20.00sec_-14.90C_LIGHT_0050.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.ugzGNHx6WC (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_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits 567.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits' -> 'wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
WCS_IMAGE_NAME=wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
WCS-calibrated image found: wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
Checking if the catalog wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits.cat corresponding to the image wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits alredy exist and is non-empty...
Catalog wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits.cat corresponding to the image wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits
WCS catalog name: wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=51, blended=18105, passed=141752
Got 141752 stars (including 123429 good ones) from the SExtractor catalog wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits.cat
util/solve_plate_with_UCAC5 got 141752 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 924.9'
Seting catalog search parameters based on the expected field of view 924.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012846 (46.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010277 (37.0 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 348.4216 through 0 to 12.6947, gap 12.6947 to 348.4216
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.2)
Done reading UCAC5 zone files...
Matched 199 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 147 matched stars entering correct_measured_positions(), 78 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 11.76"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 141 matched stars entering correct_measured_positions(), 15342 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 11.76"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 348.4333 through 0 to 12.6945, gap 12.6945 to 348.4333
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 708 (Dec 39.9 to 51.2)
Done reading UCAC5 zone files...
Matched 222 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 177 matched stars entering correct_measured_positions(), 15356 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 11.73"
Accuracy estimation diagnostic: 176 matched stars entering correct_measured_positions(), 20031 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 10.04"
Excluding outliers - 176 stars left (next iteration limit 155)
The image catalog is written to wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits -region wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_And-01-Q2b1x1_2025-12-26_19-51-17_20.00sec_-15.00C_LIGHT_0051.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.fJXwFIQv76 (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_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.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_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits
WCS_IMAGE_NAME=wcs_fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits
WCS-calibrated image found: wcs_fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits
Checking if the catalog wcs_fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits.cat corresponding to the image wcs_fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits alredy exist and is non-empty...
Catalog wcs_fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits.cat corresponding to the image wcs_fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.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_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits
WCS catalog name: wcs_fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=4530, passed=63119
Got 63119 stars (including 58509 good ones) from the SExtractor catalog wcs_fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits.cat
util/solve_plate_with_UCAC5 got 63119 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010430 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 347.4969 through 0 to 12.1405, gap 12.1405 to 347.4969
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.2 to 51.3)
Done reading UCAC5 zone files...
Matched 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 915 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 61927 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
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 347.4957 through 0 to 12.1406, gap 12.1406 to 347.4957
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.2 to 51.3)
Done reading UCAC5 zone files...
Matched 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 61925 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Accuracy estimation diagnostic: 939 matched stars entering correct_measured_positions(), 61925 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
Excluding outliers - 939 stars left (next iteration limit 1032)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits -region wcs_fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.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.8kT6W7O0AI (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_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.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_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.fits
WCS_IMAGE_NAME=wcs_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.fits
WCS-calibrated image found: wcs_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.fits
Checking if the catalog wcs_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.fits.cat corresponding to the image wcs_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.fits alredy exist and is non-empty...
Catalog wcs_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.fits.cat corresponding to the image wcs_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.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_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.fits
WCS catalog name: wcs_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=4432, passed=62235
Got 62235 stars (including 57723 good ones) from the SExtractor catalog wcs_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.fits.cat
util/solve_plate_with_UCAC5 got 62235 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010430 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 347.4973 through 0 to 12.1859, gap 12.1859 to 347.4973
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.2 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...
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 912 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 61024 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
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 347.4961 through 0 to 12.1860, gap 12.1860 to 347.4961
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.2 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
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 61026 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 61026 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.81"
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_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.fits -region wcs_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.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_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/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_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/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_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.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_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/wcs_fd_And-01-Q2b1x1_2026-04-09_06-19-42_20.00sec_-4.90C_LIGHT_0456.fits
Saving fully-calibrated image wcs_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.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_2026-04-09_CI_And-01-Q2b1x1_062112_TTUQ2b1x1_21108_PnIUokJF/wcs_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457.fits
Preparing the HTML report for the field And-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_local.txt__out118010.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161721.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161722.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__out161737.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161738.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161750.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161752.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161753.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out163278.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out164342.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out165991.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out166876.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out166897.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167113.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167195.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167583.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167822.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168283.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168457.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168520.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168765.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out168839.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169238.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169911.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169912.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out170003.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out170238.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out170394.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out170510.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out170851.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out171577.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out171873.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out171918.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out171955.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out171956.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out171973.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out172075.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out172219.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out172222.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out172245.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out172856.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173373.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173640.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173778.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173931.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173991.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out174006.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out174261.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out174333.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out174364.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out174637.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out174766.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out174846.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175171.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175188.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175297.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175386.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175483.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175717.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175991.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176126.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176256.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176334.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176528.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176766.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176893.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176899.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out176964.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177107.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177180.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out178728.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out178754.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out179157.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46096.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): 255s
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: 50s
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Considering the candidate 161721_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 161721_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
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Considering the candidate 161722_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 161722_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 161728_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 161728_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 161732_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 161732_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 161734_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 161734_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 161737_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 161737_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 161738_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 161738_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 161750_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 161750_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 161751_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
The candidate 161751_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457 did not pass the final checks
**** FOUND 00:01:48.33 +50:15:10.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 161752_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 161752_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 161753_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 161753_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 162854_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
The candidate 162854_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457 did not pass the final checks
**** FOUND 00:12:06.62 +48:12:20.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 162926_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
The candidate 162926_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457 did not pass the final checks
**** FOUND 23:45:02.51 +43:55:27.1 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 163278_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 163278_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 163917_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
The candidate 163917_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457 did not pass the final checks
**** FOUND 23:50:51.88 +43:04:44.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 164342_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 164342_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 165337_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
The candidate 165337_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457 did not pass the final checks
**** FOUND 23:40:14.75 +44:20:47.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 165991_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 165991_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166116_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
The candidate 166116_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457 did not pass the final checks
**** FOUND 23:37:22.37 +46:26:35.7 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 166544_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
The candidate 166544_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457 did not pass the final checks
**** FOUND 00:16:27.72 +43:36:54.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 166588_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
The candidate 166588_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457 did not pass the final checks
**** FOUND 23:38:07.27 +46:11:04.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 166671_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
The candidate 166671_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457 did not pass the final checks
**** FOUND 23:38:00.15 +46:13:36.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 166709_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
The candidate 166709_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457 did not pass the final checks
**** FOUND 23:42:08.41 +45:00:32.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 166876_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 166876_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166897_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 166897_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167113_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 167113_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167195_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 167195_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167547_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
The candidate 167547_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457 did not pass the final checks
**** FOUND 23:37:36.80 +44:27:14.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 167583_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 167583_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167822_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 167822_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168283_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 168283_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168457_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 168457_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168520_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 168520_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168765_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 168765_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168839_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 168839_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168925_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
The candidate 168925_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457 did not pass the final checks
**** FOUND 23:38:12.46 +43:18:00.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 169238_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 169238_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 169911_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 169911_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 169912_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 169912_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170003_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 170003_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170101_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
The candidate 170101_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457 did not pass the final checks
**** FOUND 23:37:41.25 +44:25:26.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170238_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 170238_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170394_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 170394_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170510_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 170510_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170541_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
The candidate 170541_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457 did not pass the final checks
**** FOUND 00:20:12.08 +50:06:20.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 170680_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
The candidate 170680_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457 did not pass the final checks
**** FOUND 00:11:59.87 +48:07:15.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 170851_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 170851_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171188_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
The candidate 171188_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457 did not pass the final checks
**** FOUND 00:03:20.73 +49:54:43.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171577_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 171577_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171873_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 171873_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171918_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 171918_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171955_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 171955_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171956_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 171956_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171973_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 171973_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 172075_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 172075_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 172219_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 172219_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 172222_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 172222_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 172245_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 172245_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 172339_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
The candidate 172339_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457 did not pass the final checks
**** FOUND 00:13:02.90 +49:56:53.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 172856_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 172856_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173373_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 173373_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173374_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
The candidate 173374_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457 did not pass the final checks
**** FOUND 23:55:15.48 +50:14:19.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173510_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
The candidate 173510_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457 did not pass the final checks
**** FOUND 23:37:33.87 +44:24:05.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173640_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 173640_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173677_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
The candidate 173677_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457 did not pass the final checks
**** FOUND 00:17:34.76 +49:43:58.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173778_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 173778_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173931_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 173931_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173991_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 173991_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 174006_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 174006_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 174261_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 174261_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 174333_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 174333_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 174364_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 174364_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 174636_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
The candidate 174636_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457 did not pass the final checks
**** FOUND 00:04:16.79 +49:58:41.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 174637_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 174637_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 174766_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 174766_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 174846_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 174846_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 175171_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 175171_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 175188_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 175188_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 175297_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 175297_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 175386_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 175386_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 175483_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 175483_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 175717_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 175717_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 175787_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
The candidate 175787_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457 did not pass the final checks
**** FOUND 23:44:31.70 +50:03:11.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 175991_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 175991_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 176126_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 176126_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 176256_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 176256_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 176291_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
The candidate 176291_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457 did not pass the final checks
**** FOUND 00:17:17.02 +47:55:43.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 176334_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 176334_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 176528_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 176528_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 176766_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 176766_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 176893_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 176893_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 176899_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 176899_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 176964_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 176964_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177107_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 177107_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177180_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 177180_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178728_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 178728_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178754_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 178754_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 179157_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 179157_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52886_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 52886_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 91789_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 91789_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46096_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 46096_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137188_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
The candidate 137188_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457 did not pass the final checks
**** FOUND 00:22:04.72 +44:08:42.5 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 59955_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 59955_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 77205_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 77205_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118010_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 118010_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 117622_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
The candidate 117622_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457 did not pass the final checks
**** FOUND 00:04:30.65 +42:07:13.7 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57324_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
Preparing report for the candidate 57324_fd_And-01-Q2b1x1_2026-04-09_06-20-33_20.00sec_-5.00C_LIGHT_0457
make_report_in_HTML.sh Phase 2 (HTML assembly): 4s
make_report_in_HTML.sh TOTAL: 309s
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 ####
00:22:05.02 +44:08:44.1
00:12:06.68 +48:12:20.2
23:45:02.52 +43:55:27.3
23:50:51.95 +43:04:44.2
23:54:35.04 +43:11:17.0
23:55:55.14 +49:31:44.9
23:44:27.05 +49:42:04.2
23:51:51.55 +48:26:39.8
23:37:29.56 +49:59:54.6
23:43:33.14 +50:00:46.1
23:48:52.09 +42:06:29.8
00:03:05.30 +49:49:28.5
00:14:41.90 +46:51:20.2
23:48:42.64 +46:14:34.6
23:38:24.83 +47:25:52.6
23:57:30.24 +48:17:25.2
23:41:22.67 +46:52:23.6
23:51:58.95 +49:01:25.7
23:46:23.33 +49:27:14.6
23:48:29.60 +46:16:21.7
23:40:10.87 +45:02:53.2
00:06:03.38 +49:37:35.0
23:42:09.53 +44:44:16.1
23:56:39.19 +48:26:57.1
23:50:37.81 +47:30:33.0
23:47:35.34 +49:58:04.0
00:10:16.82 +49:00:01.6
00:15:45.53 +45:30:22.8
00:05:31.31 +48:29:22.5
23:45:20.74 +44:17:42.8
00:02:09.77 +42:08:06.7
00:16:05.80 +46:59:38.2
23:39:25.64 +45:44:14.3
23:48:13.17 +47:05:59.5
23:54:25.40 +48:54:44.4
00:24:01.80 +44:14:42.1
00:24:07.63 +46:17:09.1
00:01:42.34 +46:36:22.7
23:43:17.92 +43:21:01.1
23:40:11.23 +48:47:39.8
00:17:32.51 +50:15:57.9
00:18:30.34 +43:59:38.6
00:17:36.21 +50:17:52.5
00:09:56.38 +46:22:43.5
23:52:22.08 +48:28:25.5
00:05:48.56 +45:47:22.6
23:36:51.82 +43:17:16.3
23:43:31.98 +47:19:19.4
23:46:58.79 +48:49:35.9
23:55:37.90 +48:37:56.0
23:34:39.48 +48:12:03.6
23:45:05.07 +49:44:13.1
23:40:08.70 +49:47:06.9
23:50:07.59 +47:35:53.9
23:48:38.73 +43:37:24.9
00:04:42.68 +47:25:08.1
23:41:54.48 +49:26:18.6
23:54:01.90 +44:33:36.0
23:43:26.66 +47:19:49.1
23:43:18.75 +43:20:17.7
00:01:32.01 +47:56:38.0
23:42:58.04 +47:13:12.6
00:10:11.74 +47:19:03.0
23:48:35.97 +46:15:51.3
00:01:22.46 +46:44:46.4
00:06:30.39 +47:25:01.3
23:57:20.51 +48:06:20.6
23:54:57.59 +46:52:39.2
23:37:54.57 +43:22:54.4
00:08:25.19 +44:57:38.4
00:05:50.14 +49:36:52.2
00:02:17.32 +44:32:06.8
00:03:11.41 +45:52:59.3
23:35:06.08 +47:31:15.9
00:02:46.17 +47:14:34.9
00:05:30.40 +46:40:47.2
23:51:40.59 +50:05:54.1
23:53:47.74 +50:06:37.2
23:44:49.93 +44:01:25.8
23:35:22.79 +45:57:50.1
00:10:54.95 +48:15:31.7
00:19:50.11 +47:42:37.4
23:39:51.85 +47:45:01.7
23:50:36.04 +47:31:26.4
23:34:07.44 +46:20:02.8
00:21:48.80 +44:52:18.4
########### 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 ####
00:12:06.68 +48:12:20.2
23:45:02.52 +43:55:27.3
23:50:51.95 +43:04:44.2
00:22:05.02 +44:08:44.1
23:55:55.14 +49:31:44.9
23:44:27.05 +49:42:04.2
23:51:51.55 +48:26:39.8
23:37:29.56 +49:59:54.6
23:43:33.14 +50:00:46.1
23:48:52.09 +42:06:29.8
00:03:05.30 +49:49:28.5
00:14:41.90 +46:51:20.2
23:48:42.64 +46:14:34.6
23:38:24.83 +47:25:52.6
23:57:30.24 +48:17:25.2
23:41:22.67 +46:52:23.6
23:51:58.95 +49:01:25.7
23:46:23.33 +49:27:14.6
23:48:29.60 +46:16:21.7
23:40:10.87 +45:02:53.2
00:06:03.38 +49:37:35.0
23:42:09.53 +44:44:16.1
23:56:39.19 +48:26:57.1
23:50:37.81 +47:30:33.0
23:47:35.34 +49:58:04.0
00:10:16.82 +49:00:01.6
00:15:45.53 +45:30:22.8
00:05:31.31 +48:29:22.5
23:45:20.74 +44:17:42.8
00:02:09.77 +42:08:06.7
00:16:05.80 +46:59:38.2
23:39:25.64 +45:44:14.3
23:48:13.17 +47:05:59.5
23:54:25.40 +48:54:44.4
00:24:01.80 +44:14:42.1
00:24:07.63 +46:17:09.1
00:01:42.34 +46:36:22.7
23:43:17.92 +43:21:01.1
23:40:11.23 +48:47:39.8
00:17:32.51 +50:15:57.9
00:18:30.34 +43:59:38.6
00:17:36.21 +50:17:52.5
00:09:56.38 +46:22:43.5
23:52:22.08 +48:28:25.5
00:05:48.56 +45:47:22.6
23:36:51.82 +43:17:16.3
23:43:31.98 +47:19:19.4
23:46:58.79 +48:49:35.9
23:55:37.90 +48:37:56.0
23:34:39.48 +48:12:03.6
23:45:05.07 +49:44:13.1
23:40:08.70 +49:47:06.9
23:50:07.59 +47:35:53.9
23:48:38.73 +43:37:24.9
00:04:42.68 +47:25:08.1
23:41:54.48 +49:26:18.6
23:54:01.90 +44:33:36.0
23:43:26.66 +47:19:49.1
23:43:18.75 +43:20:17.7
00:01:32.01 +47:56:38.0
23:42:58.04 +47:13:12.6
00:10:11.74 +47:19:03.0
23:48:35.97 +46:15:51.3
00:01:22.46 +46:44:46.4
00:06:30.39 +47:25:01.3
23:57:20.51 +48:06:20.6
23:54:57.59 +46:52:39.2
23:37:54.57 +43:22:54.4
00:08:25.19 +44:57:38.4
00:05:50.14 +49:36:52.2
00:02:17.32 +44:32:06.8
00:03:11.41 +45:52:59.3
23:35:06.08 +47:31:15.9
00:02:46.17 +47:14:34.9
00:05:30.40 +46:40:47.2
23:51:40.59 +50:05:54.1
23:53:47.74 +50:06:37.2
23:44:49.93 +44:01:25.8
23:35:22.79 +45:57:50.1
00:19:50.11 +47:42:37.4
00:21:48.80 +44:52:18.4
00:10:54.95 +48:15:31.7
23:50:36.04 +47:31:26.4
23:34:07.44 +46:20:02.8
23:54:35.04 +43:11:17.0
23:39:51.85 +47:45:01.7
###################################################################################
00:12:06.68 +48:12:20.2 -- not an asteroid (will add it to exclusion list)
23:45:02.52 +43:55:27.3 -- not an asteroid (will add it to exclusion list)
23:50:51.95 +43:04:44.2 -- not an asteroid (will add it to exclusion list)
00:22:05.02 +44:08:44.1 -- not an asteroid (will add it to exclusion list)
23:55:55.14 +49:31:44.9 -- not an asteroid (will add it to exclusion list)
23:44:27.05 +49:42:04.2 -- not an asteroid (will add it to exclusion list)
23:51:51.55 +48:26:39.8 -- not an asteroid (will add it to exclusion list)
23:37:29.56 +49:59:54.6 -- not an asteroid (will add it to exclusion list)
23:43:33.14 +50:00:46.1 -- not an asteroid (will add it to exclusion list)
23:48:52.09 +42:06:29.8 -- not an asteroid (will add it to exclusion list)
00:03:05.30 +49:49:28.5 -- not an asteroid (will add it to exclusion list)
00:14:41.90 +46:51:20.2 -- not an asteroid (will add it to exclusion list)
23:48:42.64 +46:14:34.6 -- not an asteroid (will add it to exclusion list)
23:38:24.83 +47:25:52.6 -- not an asteroid (will add it to exclusion list)
23:57:30.24 +48:17:25.2 -- not an asteroid (will add it to exclusion list)
23:41:22.67 +46:52:23.6 -- not an asteroid (will add it to exclusion list)
23:51:58.95 +49:01:25.7 -- not an asteroid (will add it to exclusion list)
23:46:23.33 +49:27:14.6 -- not an asteroid (will add it to exclusion list)
23:48:29.60 +46:16:21.7 -- not an asteroid (will add it to exclusion list)
23:40:10.87 +45:02:53.2 -- not an asteroid (will add it to exclusion list)
00:06:03.38 +49:37:35.0 -- not an asteroid (will add it to exclusion list)
23:42:09.53 +44:44:16.1 -- not an asteroid (will add it to exclusion list)
23:56:39.19 +48:26:57.1 -- not an asteroid (will add it to exclusion list)
23:50:37.81 +47:30:33.0 -- not an asteroid (will add it to exclusion list)
23:47:35.34 +49:58:04.0 -- not an asteroid (will add it to exclusion list)
00:10:16.82 +49:00:01.6 -- not an asteroid (will add it to exclusion list)
00:15:45.53 +45:30:22.8 -- not an asteroid (will add it to exclusion list)
00:05:31.31 +48:29:22.5 -- not an asteroid (will add it to exclusion list)
23:45:20.74 +44:17:42.8 -- not an asteroid (will add it to exclusion list)
00:02:09.77 +42:08:06.7 -- not an asteroid (will add it to exclusion list)
00:16:05.80 +46:59:38.2 -- not an asteroid (will add it to exclusion list)
23:39:25.64 +45:44:14.3 -- not an asteroid (will add it to exclusion list)
23:48:13.17 +47:05:59.5 -- not an asteroid (will add it to exclusion list)
23:54:25.40 +48:54:44.4 -- not an asteroid (will add it to exclusion list)
00:24:01.80 +44:14:42.1 -- not an asteroid (will add it to exclusion list)
00:24:07.63 +46:17:09.1 -- not an asteroid (will add it to exclusion list)
00:01:42.34 +46:36:22.7 -- not an asteroid (will add it to exclusion list)
23:43:17.92 +43:21:01.1 -- not an asteroid (will add it to exclusion list)
23:40:11.23 +48:47:39.8 -- not an asteroid (will add it to exclusion list)
00:17:32.51 +50:15:57.9 -- not an asteroid (will add it to exclusion list)
00:18:30.34 +43:59:38.6 -- not an asteroid (will add it to exclusion list)
00:17:36.21 +50:17:52.5 -- not an asteroid (will add it to exclusion list)
00:09:56.38 +46:22:43.5 -- not an asteroid (will add it to exclusion list)
23:52:22.08 +48:28:25.5 -- not an asteroid (will add it to exclusion list)
00:05:48.56 +45:47:22.6 -- not an asteroid (will add it to exclusion list)
23:36:51.82 +43:17:16.3 -- not an asteroid (will add it to exclusion list)
23:43:31.98 +47:19:19.4 -- not an asteroid (will add it to exclusion list)
23:46:58.79 +48:49:35.9 -- not an asteroid (will add it to exclusion list)
23:55:37.90 +48:37:56.0 -- not an asteroid (will add it to exclusion list)
23:34:39.48 +48:12:03.6 -- not an asteroid (will add it to exclusion list)
23:45:05.07 +49:44:13.1 -- not an asteroid (will add it to exclusion list)
23:40:08.70 +49:47:06.9 -- not an asteroid (will add it to exclusion list)
23:50:07.59 +47:35:53.9 -- not an asteroid (will add it to exclusion list)
23:48:38.73 +43:37:24.9 -- not an asteroid (will add it to exclusion list)
00:04:42.68 +47:25:08.1 -- not an asteroid (will add it to exclusion list)
23:41:54.48 +49:26:18.6 -- not an asteroid (will add it to exclusion list)
23:54:01.90 +44:33:36.0 -- not an asteroid (will add it to exclusion list)
23:43:26.66 +47:19:49.1 -- not an asteroid (will add it to exclusion list)
23:43:18.75 +43:20:17.7 -- not an asteroid (will add it to exclusion list)
00:01:32.01 +47:56:38.0 -- not an asteroid (will add it to exclusion list)
23:42:58.04 +47:13:12.6 -- not an asteroid (will add it to exclusion list)
00:10:11.74 +47:19:03.0 -- not an asteroid (will add it to exclusion list)
23:48:35.97 +46:15:51.3 -- not an asteroid (will add it to exclusion list)
00:01:22.46 +46:44:46.4 -- not an asteroid (will add it to exclusion list)
00:06:30.39 +47:25:01.3 -- not an asteroid (will add it to exclusion list)
23:57:20.51 +48:06:20.6 -- not an asteroid (will add it to exclusion list)
23:54:57.59 +46:52:39.2 -- not an asteroid (will add it to exclusion list)
23:37:54.57 +43:22:54.4 -- not an asteroid (will add it to exclusion list)
00:08:25.19 +44:57:38.4 -- not an asteroid (will add it to exclusion list)
00:05:50.14 +49:36:52.2 -- not an asteroid (will add it to exclusion list)
00:02:17.32 +44:32:06.8 -- not an asteroid (will add it to exclusion list)
00:03:11.41 +45:52:59.3 -- not an asteroid (will add it to exclusion list)
23:35:06.08 +47:31:15.9 -- not an asteroid (will add it to exclusion list)
00:02:46.17 +47:14:34.9 -- not an asteroid (will add it to exclusion list)
00:05:30.40 +46:40:47.2 -- not an asteroid (will add it to exclusion list)
23:51:40.59 +50:05:54.1 -- not an asteroid (will add it to exclusion list)
23:53:47.74 +50:06:37.2 -- not an asteroid (will add it to exclusion list)
23:44:49.93 +44:01:25.8 -- not an asteroid (will add it to exclusion list)
23:35:22.79 +45:57:50.1 -- not an asteroid (will add it to exclusion list)
00:19:50.11 +47:42:37.4 -- not an asteroid (will add it to exclusion list)
00:21:48.80 +44:52:18.4 -- not an asteroid (will add it to exclusion list)
00:10:54.95 +48:15:31.7 -- not an asteroid (will add it to exclusion list)
23:50:36.04 +47:31:26.4 -- not an asteroid (will add it to exclusion list)
23:34:07.44 +46:20:02.8 -- not an asteroid (will add it to exclusion list)
23:54:35.04 +43:11:17.0 -- not an asteroid (will add it to exclusion list)
23:39:51.85 +47:45:01.7 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
00:01:22.46 +46:44:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:01:32.01 +47:56:38.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:01:42.34 +46:36:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:02:09.77 +42:08:06.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:02:17.32 +44:32:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:02:46.17 +47:14:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:03:05.30 +49:49:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:03:11.41 +45:52:59.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:04:42.68 +47:25:08.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:05:30.40 +46:40:47.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:05:31.31 +48:29:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:05:48.56 +45:47:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:05:50.14 +49:36:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:06:03.38 +49:37:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:06:30.39 +47:25:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:08:25.19 +44:57:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:09:56.38 +46:22:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:10:11.74 +47:19:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:10:16.82 +49:00:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:10:54.95 +48:15:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:12:06.68 +48:12:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:14:41.90 +46:51:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:15:45.53 +45:30:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:16:05.80 +46:59:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:17:32.51 +50:15:57.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:17:36.21 +50:17:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:18:30.34 +43:59:38.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:19:50.11 +47:42:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:21:48.80 +44:52:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:22:05.02 +44:08:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:24:01.80 +44:14:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:24:07.63 +46:17:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:34:07.44 +46:20:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:34:39.48 +48:12:03.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:35:06.08 +47:31:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:35:22.79 +45:57:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:36:51.82 +43:17:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:37:29.56 +49:59:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:37:54.57 +43:22:54.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:38:24.83 +47:25:52.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:39:25.64 +45:44:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:39:51.85 +47:45:01.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:40:08.70 +49:47:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:40:10.87 +45:02:53.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:40:11.23 +48:47:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:41:22.67 +46:52:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:41:54.48 +49:26:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:42:09.53 +44:44:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:42:58.04 +47:13:12.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:43:17.92 +43:21:01.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:43:18.75 +43:20:17.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:43:26.66 +47:19:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:43:31.98 +47:19:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:43:33.14 +50:00:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:44:27.05 +49:42:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:44:49.93 +44:01:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:45:02.52 +43:55:27.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:45:05.07 +49:44:13.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:45:20.74 +44:17:42.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:46:23.33 +49:27:14.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:46:58.79 +48:49:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:47:35.34 +49:58:04.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:48:13.17 +47:05:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:48:29.60 +46:16:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:48:35.97 +46:15:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:48:38.73 +43:37:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:48:42.64 +46:14:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:48:52.09 +42:06:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:50:07.59 +47:35:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:50:36.04 +47:31:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:50:37.81 +47:30:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:50:51.95 +43:04:44.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:51:40.59 +50:05:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:51:51.55 +48:26:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:51:58.95 +49:01:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:52:22.08 +48:28:25.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:53:47.74 +50:06:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:54:01.90 +44:33:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:54:25.40 +48:54:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:54:35.04 +43:11:17.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:54:57.59 +46:52:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:55:37.90 +48:37:56.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:55:55.14 +49:31:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:56:39.19 +48:26:57.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:57:20.51 +48:06:20.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:57:30.24 +48:17:25.2 -- 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)
00:01:22.46 +46:44:46.4 -- not a known variable star
00:01:32.01 +47:56:38.0 -- not a known variable star
00:01:42.34 +46:36:22.7 -- not a known variable star
00:02:09.77 +42:08:06.7 -- not a known variable star
00:02:17.32 +44:32:06.8 -- not a known variable star
00:02:46.17 +47:14:34.9 -- not a known variable star
00:03:05.30 +49:49:28.5 -- not a known variable star
00:03:11.41 +45:52:59.3 -- not a known variable star
00:04:42.68 +47:25:08.1 -- not a known variable star
00:05:30.40 +46:40:47.2 -- not a known variable star
00:05:31.31 +48:29:22.5 -- not a known variable star
00:05:48.56 +45:47:22.6 -- not a known variable star
00:05:50.14 +49:36:52.2 -- not a known variable star
00:06:03.38 +49:37:35.0 -- not a known variable star
00:06:30.39 +47:25:01.3 -- a known variable star
00:08:25.19 +44:57:38.4 -- not a known variable star
00:09:56.38 +46:22:43.5 -- not a known variable star
00:10:11.74 +47:19:03.0 -- not a known variable star
00:10:16.82 +49:00:01.6 -- a known variable star
00:10:54.95 +48:15:31.7 -- a known variable star
00:12:06.68 +48:12:20.2 -- a known variable star
00:14:41.90 +46:51:20.2 -- not a known variable star
00:15:45.53 +45:30:22.8 -- not a known variable star
00:16:05.80 +46:59:38.2 -- not a known variable star
00:17:32.51 +50:15:57.9 -- not a known variable star
00:17:36.21 +50:17:52.5 -- not a known variable star
00:18:30.34 +43:59:38.6 -- not a known variable star
00:19:50.11 +47:42:37.4 -- a known variable star
00:21:48.80 +44:52:18.4 -- a known variable star
00:22:05.02 +44:08:44.1 -- a known variable star
00:24:01.80 +44:14:42.1 -- not a known variable star
00:24:07.63 +46:17:09.1 -- not a known variable star
23:34:07.44 +46:20:02.8 -- a known variable star
23:34:39.48 +48:12:03.6 -- not a known variable star
23:35:06.08 +47:31:15.9 -- not a known variable star
23:35:22.79 +45:57:50.1 -- not a known variable star
23:36:51.82 +43:17:16.3 -- not a known variable star
23:37:29.56 +49:59:54.6 -- not a known variable star
23:37:54.57 +43:22:54.4 -- not a known variable star
23:38:24.83 +47:25:52.6 -- a known variable star
23:39:25.64 +45:44:14.3 -- not a known variable star
23:39:51.85 +47:45:01.7 -- a known variable star
23:40:08.70 +49:47:06.9 -- not a known variable star
23:40:10.87 +45:02:53.2 -- not a known variable star
23:40:11.23 +48:47:39.8 -- a known variable star
23:41:22.67 +46:52:23.6 -- not a known variable star
23:41:54.48 +49:26:18.6 -- not a known variable star
23:42:09.53 +44:44:16.1 -- not a known variable star
23:42:58.04 +47:13:12.6 -- not a known variable star
23:43:17.92 +43:21:01.1 -- not a known variable star
23:43:18.75 +43:20:17.7 -- not a known variable star
23:43:26.66 +47:19:49.1 -- not a known variable star
23:43:31.98 +47:19:19.4 -- not a known variable star
23:43:33.14 +50:00:46.1 -- not a known variable star
23:44:27.05 +49:42:04.2 -- not a known variable star
23:44:49.93 +44:01:25.8 -- not a known variable star
23:45:02.52 +43:55:27.3 -- a known variable star
23:45:05.07 +49:44:13.1 -- not a known variable star
23:45:20.74 +44:17:42.8 -- not a known variable star
23:46:23.33 +49:27:14.6 -- not a known variable star
23:46:58.79 +48:49:35.9 -- a known variable star
23:47:35.34 +49:58:04.0 -- not a known variable star
23:48:13.17 +47:05:59.5 -- not a known variable star
23:48:29.60 +46:16:21.7 -- not a known variable star
23:48:35.97 +46:15:51.3 -- not a known variable star
23:48:38.73 +43:37:24.9 -- a known variable star
23:48:42.64 +46:14:34.6 -- not a known variable star
23:48:52.09 +42:06:29.8 -- a known variable star
23:50:07.59 +47:35:53.9 -- not a known variable star
23:50:36.04 +47:31:26.4 -- not a known variable star
23:50:37.81 +47:30:33.0 -- not a known variable star
23:50:51.95 +43:04:44.2 -- a known variable star
23:51:40.59 +50:05:54.1 -- not a known variable star
23:51:51.55 +48:26:39.8 -- not a known variable star
23:51:58.95 +49:01:25.7 -- not a known variable star
23:52:22.08 +48:28:25.5 -- not a known variable star
23:53:47.74 +50:06:37.2 -- not a known variable star
23:54:01.90 +44:33:36.0 -- not a known variable star
23:54:25.40 +48:54:44.4 -- not a known variable star
23:54:35.04 +43:11:17.0 -- a known variable star
23:54:57.59 +46:52:39.2 -- not a known variable star
23:55:37.90 +48:37:56.0 -- not a known variable star
23:55:55.14 +49:31:44.9 -- not a known variable star
23:56:39.19 +48:26:57.1 -- not a known variable star
23:57:20.51 +48:06:20.6 -- not a known variable star
23:57:30.24 +48:17:25.2 -- a known variable star
Found 68 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
86 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 86 (excluding asteroids and hot pixels, 68 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)2461139.97214101 -observatory V36
23:34:54.56 -05:12:46.3 Mercury (0.2mag)
02:37:05.49 +15:15:34.8 Venus (-3.9mag)
23:59:16.37 -01:10:50.9 Mars (1.2mag)
07:09:53.73 +22:50:35.9 Jupiter (-2.1mag)
00:26:15.02 +00:30:36.7 Saturn (0.9mag)
03:46:21.70 +19:43:10.1 Uranus (5.8mag)
00:09:58.45 -00:20:51.0 Neptune (7.8mag)
20:33:25.79 -22:52:27.0 Pluto (14.5mag)
18:51:26.12 -28:01:51.3 Moon (-10.6mag)
-rw-r--r-- 1 apache apache 362 Apr 9 06:22 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461139.97214101:
07:10:01.72 +22:50:19.5 Io (5.7mag)
07:10:05.93 +22:50:11.6 Europa (5.9mag)
07:10:04.40 +22:50:08.0 Ganymede (5.3mag)
07:09:25.49 +22:51:37.1 Callisto (6.5mag)
07:13:29.90 +22:41:24.1 Himalia (15.3mag)
07:09:49.69 +22:50:44.0 Thebe (16.2mag)
07:13:32.37 +23:10:48.9 Elara (17.3mag)
07:08:19.98 +23:34:01.2 Pasiphae (17.4mag)
07:18:21.75 +22:47:55.6 Carme (18.5mag)
00:26:22.78 +00:30:26.1 Titan (8.8mag)
00:26:18.21 +00:30:48.8 Rhea (10.1mag)
00:26:08.12 +00:31:45.6 Iapetus (11.5mag)
00:26:27.11 +00:30:23.6 Hyperion (14.8mag)
00:27:56.90 +00:40:06.1 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 9 06:22 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461139.97214101:
15:04:49.33 -11:14:28.0 JWST
17:55:55.52 +35:29:07.7 Chandra
20:16:10.66 +25:49:50.8 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 9 06:22 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461139.97214101 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:48:57.41 -28:24:37.4 13.9mag P/2010 H2 (Vales)
05:02:12.91 -69:58:48.8 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:31:08.34 +31:23:42.7 17.2mag C/2017 K2 (PANSTARRS)
17:30:52.91 +09:46:02.0 17.6mag C/2021 G2 (ATLAS)
23:08:22.49 +28:58:54.5 17.0mag C/2022 E2 (ATLAS)
04:21:42.52 +25:51:27.3 15.9mag C/2022 N2 (PANSTARRS)
09:02:15.18 +31:57:23.1 16.2mag C/2022 QE78 (ATLAS)
08:30:14.93 -00:51:43.2 17.3mag C/2022 R6 (PANSTARRS)
18:55:04.73 +17:58:41.0 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:42:38.69 -11:36:56.0 17.6mag P/2023 B1 (PANSTARRS)
09:10:56.25 -12:57:00.5 17.6mag C/2023 F3 (ATLAS)
21:47:16.84 +62:32:27.4 17.5mag C/2023 H5 (Lemmon)
19:24:17.43 -03:38:30.7 14.2mag C/2023 R1 (PANSTARRS)
21:41:06.82 +85:01:48.8 17.8mag C/2023 X2 (Lemmon)
06:15:21.80 +63:33:12.2 17.1mag C/2024 A1 (ATLAS)
04:58:47.82 +15:56:03.2 10.6mag C/2024 E1 (Wierzchos)
16:23:16.22 +05:19:03.4 17.4mag C/2024 G6 (ATLAS)
20:18:45.61 +13:31:56.8 14.7mag C/2024 J3 (ATLAS)
03:20:35.64 -23:23:53.3 16.4mag C/2024 T5 (ATLAS)
05:11:18.27 +46:57:24.0 17.7mag C/2025 J1 (Borisov)
14:05:52.33 +40:30:11.9 14.9mag C/2025 L1 (ATLAS)
03:15:12.94 -25:13:21.2 17.8mag C/2025 Q3 (ATLAS)
23:03:56.31 +19:45:25.9 9.6mag C/2025 R3 (PANSTARRS)
12:56:57.57 +02:36:18.2 17.5mag C/2025 Y1 (ATLAS)
02:21:12.66 +03:39:39.4 10.5mag C/2026 A1 (MAPS)
23:40:39.84 +35:56:50.5 14.4mag C/2026 B2 (Sun-Gao)
18:30:12.08 -10:03:33.3 12.2mag 10P/Tempel
15:08:53.19 +03:50:17.2 13.4mag 24P/Schaumasse
11:04:41.78 -01:44:46.0 15.7mag 29P/Schwassmann-Wachmann
17:58:29.37 -09:51:38.8 17.8mag 40P/Vaisala
10:38:13.15 -04:38:52.8 16.8mag 43P/Wolf-Harrington
01:38:35.78 +16:21:59.9 17.2mag 47P/Ashbrook-Jackson
06:58:59.52 +38:23:51.3 17.0mag 63P/Wild
23:20:37.93 -12:14:46.7 15.7mag 65P/Gunn
03:46:04.75 +18:56:55.3 15.9mag 76P/West-Kohoutek-Ikemura
00:51:13.48 +06:56:19.1 14.4mag 78P/Gehrels
22:42:55.26 -11:18:55.7 14.6mag 88P/Howell
01:52:09.13 +18:52:01.9 15.1mag 93P/Lovas
04:42:45.35 +31:55:24.5 16.3mag 123P/West-Hartley
08:21:07.92 +41:22:27.8 16.2mag 124P/Mrkos
02:23:11.73 +13:38:01.2 16.4mag 128P/Shoemaker-Holt
02:34:46.54 +13:40:42.7 17.5mag 131P/Mueller
00:52:22.75 +10:52:28.8 11.0mag 141P/Machholz
01:02:05.24 +02:25:18.8 11.0mag 141P-A/Machholz
23:50:46.10 -01:22:55.5 13.6mag 141P-D/Machholz
01:31:42.25 +04:08:03.7 17.9mag 141P-I/Machholz
00:44:13.62 -04:47:38.3 15.2mag 162P/SidingSpring
10:30:01.28 +31:17:58.2 17.9mag 164P/Christensen
06:24:26.94 +24:26:26.5 17.9mag 198P/ODAS
15:02:59.71 -00:47:34.1 17.4mag 210P/Christensen
21:19:18.30 -13:01:43.7 17.5mag 218P/LINEAR
17:14:17.06 -14:42:10.7 16.2mag 235P/LINEAR
05:20:32.00 +34:09:42.2 16.6mag 240P/NEAT
07:35:30.32 -05:53:54.8 17.7mag 242P/Spahr
15:44:58.01 +06:32:40.6 17.5mag 391P/Kowalski
07:31:53.61 +21:20:07.9 17.6mag 450P/LONEOS
05:26:29.68 +45:24:57.3 17.5mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 9 06:22 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.70 -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
12:20:27.96 -45:55:38.40 ASASSN-26bt 2026-03-18.8 16.32
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
13:01:19.46 +15:42:15.50 SN2026ehe 2026-03-12.34 -0.18
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.70 -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
14:15:47.49 -48:05:16.60 SN2026dez 2026-02-19.31 15.91
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
-rw-r--r-- 1 apache apache 5.8K Apr 9 06:22 asassn_transients_list.txt
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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 9 06:22 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
16:19:43.830 +52:24:20.17 AT 2026igg 2026-03-30.82 20.61
16:02:50.720 +53:43:35.02 AT 2026igf 2026-03-30.82 20.66
15:41:26.040 +51:39:22.68 AT 2026ige 2026-03-30.82 21.55
15:46:44.960 +52:41:18.17 AT 2026igd 2026-03-30.82 20.83
16:01:16.770 +47:31:43.64 AT 2026igc 2026-03-30.81 21.19
16:25:08.810 +44:48:12.28 AT 2026igb 2026-03-30.81 21.33
16:13:40.950 +40:54:21.62 AT 2026iga 2026-03-30.81 20.28
15:50:48.070 +48:03:43.08 AT 2026ifz 2026-03-30.81 20.51
15:50:43.720 +47:30:42.19 AT 2026ify 2026-03-30.81 21.34
17:38:02.570 +25:54:11.91 AT 2026ifx 2026-03-27.88 20.89
16:42:02.490 +40:59:30.50 AT 2026ifw 2026-03-27.86 21.32
16:24:14.050 +39:37:35.59 AT 2026ifv 2026-03-27.86 20.81
16:16:45.660 +38:01:36.33 AT 2026ifu 2026-03-27.86 21.15
16:28:23.190 +36:11:26.67 AT 2026ift 2026-03-27.86 21.53
16:16:10.610 +36:40:26.87 AT 2026ifs 2026-03-27.86 20.03
16:42:08.700 +33:28:34.26 AT 2026ifr 2026-03-27.86 21.24
16:45:41.760 +34:10:06.31 AT 2026ifq 2026-03-27.86 21.64
16:50:17.550 +33:04:52.33 AT 2026ifp 2026-03-27.86 19.99
16:52:21.140 +31:25:32.03 AT 2026ifo 2026-03-27.86 19.73
16:06:48.970 +28:22:45.47 AT 2026ifn 2026-03-27.85 21.37
-rw-r--r-- 1 apache apache 30K Apr 9 06:22 tns_transients_list.txt
