This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx
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 02.4449* 00 20 13.72 +62 07 34.6 9.4 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
CU Cas,2461132.9449,9.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CU Cas 20260402.4449 9.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 00 35 02.21 +61 18 56.2 10.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0826 Cas,2461132.9449,10.67,0.05,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
V0826 Cas 20260402.4449 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 02.4449* 00 29 19.95 +60 02 41.7 12.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 428524903065972224,2461132.9449,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 428524903065972224 20260402.4449 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 00 57 01.27 +65 41 58.3 12.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 525886176663536256,2461132.9449,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 525886176663536256 20260402.4449 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 00 56 30.28 +65 09 58.8 11.4 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 524358851937425792,2461132.9449,11.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 524358851937425792 20260402.4449 11.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 00 57 01.45 +65 37 03.3 11.4 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 525885420749318016,2461132.9449,11.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 525885420749318016 20260402.4449 11.41CV 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 02.4449* 23 24 21.41 +61 36 20.7 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461132.9449,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260402.4449 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 23 46 05.16 +62 40 58.5 12.8 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2015981782442688768,2461132.9449,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2015981782442688768 20260402.4449 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 00 15 07.55 +66 20 31.6 13.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0015065+662031,2461132.9449,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0015065+662031 20260402.4449 13.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 00 52 22.45 +65 13 14.3 13.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J005223.00+651320.3,2461132.9449,13.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J005223.00+651320.3 20260402.4449 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 00 34 25.82 +64 32 50.4 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0660 Cas,2461132.9449,11.81,0.05,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
V0660 Cas 20260402.4449 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 02.4449* 00 35 52.83 +60 37 12.8 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J003553.23+603714.5,2461132.9449,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J003553.23+603714.5 20260402.4449 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 00 45 33.47 +60 31 45.7 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J004533.91+603145.5,2461132.9449,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J004533.91+603145.5 20260402.4449 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 23 48 02.00 +62 37 47.5 13.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 1490642,2461132.9449,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 1490642 20260402.4449 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 00 22 55.50 +64 31 43.0 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 1657339,2461132.9449,11.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 1657339 20260402.4449 11.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 23 46 09.44 +61 12 19.7 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 1488936,2461132.9449,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 1488936 20260402.4449 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 23 48 14.14 +61 01 54.1 10.8 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
EM Cas,2461132.9449,10.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
EM Cas 20260402.4449 10.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 00 52 02.98 +62 24 45.3 12.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 523615238482462336,2461132.9449,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 523615238482462336 20260402.4449 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 00 04 06.97 +60 48 51.1 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSV 15008,2461132.9449,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 15008 20260402.4449 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 00 18 46.99 +59 05 05.1 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 1566905,2461132.9449,11.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 1566905 20260402.4449 11.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 00 31 19.62 +59 18 28.1 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J003119.85+591827.0,2461132.9449,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J003119.85+591827.0 20260402.4449 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 00 08 21.87 +60 36 43.0 12.8 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 1611272,2461132.9449,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 1611272 20260402.4449 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 00 48 55.20 +61 24 40.1 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0048554+612440,2461132.9449,11.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0048554+612440 20260402.4449 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 00 40 05.18 +60 01 37.1 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 1634390,2461132.9449,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 1634390 20260402.4449 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 00 04 10.80 +60 55 22.0 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J000410.84+605522.3,2461132.9449,10.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J000410.84+605522.3 20260402.4449 10.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 00 41 24.03 +61 33 20.4 12.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSV 256,2461132.9449,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 256 20260402.4449 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 23 47 21.51 +58 13 17.1 9.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
TYC 4013-648-1,2461132.9449,9.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
TYC 4013-648-1 20260402.4449 9.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 00 28 33.50 +59 15 27.4 12.8 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
MNIC V9,2461132.9449,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
MNIC V9 20260402.4449 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 00 27 28.62 +59 19 49.1 10.8 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSV 15096,2461132.9449,10.79,0.05,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
NSV 15096 20260402.4449 10.79CV 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 02.4449* 00 41 49.42 +61 28 42.8 10.8 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSV 257,2461132.9449,10.83,0.05,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
NSV 257 20260402.4449 10.83CV 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 02.4449* 23 54 36.76 +58 43 43.1 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J235436.58+584343.5,2461132.9449,12.31,0.05,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
ASASSN-V J235436.58+584343.5 20260402.4449 12.31CV 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 02.4449* 00 40 44.39 +62 05 03.5 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J004045.00+620505.3,2461132.9449,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J004045.00+620505.3 20260402.4449 11.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 23 56 17.94 +58 01 20.2 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2356179+580117,2461132.9449,12.87,0.05,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
NSVS J2356179+580117 20260402.4449 12.87CV 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 02.4449* 23 57 22.05 +62 10 57.8 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
QV Cas,2461132.9449,12.06,0.05,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
QV Cas 20260402.4449 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 02.4449* 00 37 01.48 +61 25 08.5 12.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
CzeV4227,2461132.9449,12.23,0.05,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
CzeV4227 20260402.4449 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 02.4449* 00 10 53.44 +63 51 21.1 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0010537+635124,2461132.9449,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0010537+635124 20260402.4449 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 00 27 56.89 +65 26 12.0 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
USNO-B1.0 1554-008230,2461132.9449,11.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
USNO-B1.0 1554-008230 20260402.4449 11.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 23 47 12.55 +58 54 15.5 12.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461132.9449,12.33,0.05,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
VARIABLE_NAME 20260402.4449 12.33CV 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 02.4449* 00 05 32.74 +63 52 38.5 13.0 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J000532.56+635242.7,2461132.9449,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J000532.56+635242.7 20260402.4449 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 00 48 32.67 +62 04 22.0 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 1670275,2461132.9449,11.57,0.05,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
NSVS 1670275 20260402.4449 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 02.4449* 00 35 25.34 +61 14 41.2 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1302 Cas,2461132.9449,11.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1302 Cas 20260402.4449 11.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 00 28 08.17 +60 29 29.8 11.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSV 168,2461132.9449,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 168 20260402.4449 11.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 23 53 22.02 +59 38 43.4 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J235321.78+593844.9,2461132.9449,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J235321.78+593844.9 20260402.4449 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 00 24 11.86 +57 57 09.9 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0024122+575706,2461132.9449,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0024122+575706 20260402.4449 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 23 57 21.49 +58 25 05.1 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0653 Cas,2461132.9449,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0653 Cas 20260402.4449 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 23 48 23.86 +58 50 27.9 10.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2348236+585025,2461132.9449,10.62,0.05,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
NSVS J2348236+585025 20260402.4449 10.62CV 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 02.4449* 00 39 38.72 +60 46 05.8 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSV 243,2461132.9449,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 243 20260402.4449 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 00 04 40.43 +60 22 00.6 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
FF Cas,2461132.9449,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
FF Cas 20260402.4449 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 00 15 13.34 +59 00 24.9 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
TSVSC1 TN-N311213223-279-82-2,2461132.9449,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
TSVSC1 TN-N311213223-279-82-2 20260402.4449 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 23 57 58.44 +59 25 09.8 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ET Cas,2461132.9449,12.07,0.05,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
ET Cas 20260402.4449 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 02.4449* 00 50 25.09 +63 36 02.9 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J005025.79+633605.5,2461132.9449,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J005025.79+633605.5 20260402.4449 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 23 44 25.45 +59 40 08.4 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2344252+594006,2461132.9449,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2344252+594006 20260402.4449 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 23 50 34.84 +59 27 31.0 13.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 1541803,2461132.9449,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 1541803 20260402.4449 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 00 22 51.88 +65 40 24.5 13.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 1659094,2461132.9449,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 1659094 20260402.4449 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 00 47 23.28 +62 28 01.4 11.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J004724.14+622803.6,2461132.9449,11.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J004724.14+622803.6 20260402.4449 11.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 00 12 18.99 +62 44 56.2 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J001219.05+624459.7,2461132.9449,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J001219.05+624459.7 20260402.4449 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 00 34 30.84 +61 56 40.9 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0034316+615643,2461132.9449,11.83,0.05,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
NSVS J0034316+615643 20260402.4449 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 02.4449* 23 43 06.20 +60 02 47.5 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2343062+600246,2461132.9449,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2343062+600246 20260402.4449 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 23 55 46.74 +63 04 26.3 12.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 1495775,2461132.9449,12.33,0.05,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
NSVS 1495775 20260402.4449 12.33CV 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 02.4449* 00 26 14.81 +58 05 38.3 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
SAVS 002615+580536,2461132.9449,11.99,0.05,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
SAVS 002615+580536 20260402.4449 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 02.4449* 23 37 02.31 +60 42 00.8 13.0 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2012227916604958976,2461132.9449,13.02,0.05,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
Gaia DR3 2012227916604958976 20260402.4449 13.02CV 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 02.4449* 23 39 27.28 +62 23 44.6 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSV 26121,2461132.9449,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 26121 20260402.4449 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 00 34 42.32 +65 40 07.0 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 1626030,2461132.9449,11.81,0.05,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
NSVS 1626030 20260402.4449 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 02.4449* 23 59 38.66 +59 45 29.6 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0335 Cas,2461132.9449,11.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0335 Cas 20260402.4449 11.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 00 27 09.45 +60 10 36.0 11.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J002709.83+601036.1,2461132.9449,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J002709.83+601036.1 20260402.4449 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 00 32 54.27 +58 24 23.1 12.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J003254.54+582420.6,2461132.9449,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J003254.54+582420.6 20260402.4449 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 23 54 45.03 +59 42 30.4 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2354445+594237,2461132.9449,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2354445+594237 20260402.4449 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 23 39 58.98 +63 20 52.6 11.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0441 Cas,2461132.9449,11.47,0.05,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
V0441 Cas 20260402.4449 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 02.4449* 00 49 16.80 +63 10 03.4 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J004917.60+631005.4,2461132.9449,10.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J004917.60+631005.4 20260402.4449 10.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 00 39 02.29 +61 37 11.9 12.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J003902.80+613712.6,2461132.9449,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J003902.80+613712.6 20260402.4449 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 00 52 21.15 +63 28 56.7 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0052215+632858,2461132.9449,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0052215+632858 20260402.4449 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 00 21 58.09 +61 32 43.9 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J002158.95+613245.0,2461132.9449,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J002158.95+613245.0 20260402.4449 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 00 39 01.97 +64 04 15.0 12.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J003902.46+640417.4,2461132.9449,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J003902.46+640417.4 20260402.4449 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 00 46 50.29 +60 17 46.1 11.0 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1307 Cas,2461132.9449,11.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1307 Cas 20260402.4449 11.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 00 26 06.08 +60 15 13.6 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461132.9449,12.43,0.05,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
VARIABLE_NAME 20260402.4449 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 02.4449* 23 58 43.98 +63 21 10.6 12.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J235843.80+632113.9,2461132.9449,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J235843.80+632113.9 20260402.4449 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 23 25 17.67 +60 57 31.8 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2325169+605731,2461132.9449,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2325169+605731 20260402.4449 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 00 51 25.01 +62 55 13.4 8.0 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 523666743731963136,2461132.9449,8.03,0.05,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 523666743731963136 20260402.4449 8.03CV 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 02.4449* 00 07 05.48 +61 48 53.5 11.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0658 Cas,2461132.9449,11.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0658 Cas 20260402.4449 11.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 23 52 39.24 +60 56 06.3 12.8 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J235239.22+605608.1,2461132.9449,12.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J235239.22+605608.1 20260402.4449 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 00 21 50.88 +63 25 59.9 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J002151.32+632602.2,2461132.9449,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J002151.32+632602.2 20260402.4449 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.4449* 00 30 30.39 +59 50 50.4 12.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J003030.91+595049.2,2461132.9449,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J003030.91+595049.2 20260402.4449 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461036.58829464 27.12.2025 02:06:58.657 /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
First image: 2461036.58829464 27.12.2025 02:06:58.657 /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
Last image: 2461132.94520501 02.04.2026 10:40:55.713 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 11
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.98
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): 22050
Objects passed selection criteria: 21912
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 14710.5
Average stars matched: 13929.8 (94.6926 %)
Memory usage VmPeak: 125840 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 1 15:05:04 CDT 2026
VaST build number 1.0rc88-372-gf0c1109d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-01)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 2 05:45:11 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: 2461036.58829464 27.12.2025 02:06:58.657 /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
First image: 2461036.58829464 27.12.2025 02:06:58.657 /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
Last image: 2461132.94520501 02.04.2026 10:40:55.713 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 232
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.62
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: 26 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): 144915
Objects passed selection criteria: 144508
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 99047
Average stars matched: 93045 (93.9403 %)
Memory usage VmPeak: 1906184 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 1 15:05:04 CDT 2026
VaST build number 1.0rc88-372-gf0c1109d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-01)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 2 05:47:39 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/Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits
SExtractor catalog cache: saved Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits.cat to cache
SExtractor catalog cache: saved Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.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/Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.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: 2461132.94458920
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits exists and is non-empty
Saving wcs_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits to local_wcs_cache/
'wcs_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits' -> 'local_wcs_cache/wcs_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits'
wcs_Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits exists and is non-empty
Saving wcs_Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits to local_wcs_cache/
'wcs_Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits' -> 'local_wcs_cache/wcs_Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits'
wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits exists and is non-empty
Saving wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits to local_wcs_cache/
'wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits' -> 'local_wcs_cache/wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits'
wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits exists and is non-empty
Saving wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits to local_wcs_cache/
'wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits' -> 'local_wcs_cache/wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:00:01.853 +61:59:36.76
Second-epoch image center 23:59:59.312 +62:03:48.58
Angular distance between the image centers 0.07 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 00:00:01.853 +61:59:36.76
Second-epoch image center 23:59:56.815 +62:03:20.57
Angular distance between the image centers 0.06 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 23:59:59.312 +62:03:48.58
Second-epoch second image center 23:59:56.815 +62:03:20.57
Angular distance between the image centers 0.00918 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/Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits &> /tmp/tmp.mH11wkD4dq
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits &> /tmp/tmp.5HEwGiQNCz
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits &> /tmp/tmp.dBMxIPn7lC
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits &> /tmp/tmp.rwqDJrZXoC
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.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_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits and wcs_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.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_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits and wcs_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits.cat
Found non-empty wcs_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits and wcs_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits.cat
The reference image (wcs_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits) and catalog (wcs_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits.cat) found
'wcs_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits.cat' -> 'wcsmag.cat'
Read 25547 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0005 to 359.9978 deg, Dec +55.3501 to +67.4045 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 0.0005 to 359.9978 deg, Dec 55.3501 to 67.4045 deg
Loaded 133072 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): 14110 out of 15859 total matches.
Matched with Tycho-2 15859 out of 25547 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.955169
a=0.000000 b=1.000000 c=22.955169
From vast_summary.log: estimated ref. image limiting mag.: -7.98
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.98
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.98
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 9 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.5 pix Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
2.5 pix Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits
3.2 pix fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits
3.2 pix fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits
Limiting magnitude estimates:
15.0 mag. Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
15.0 mag. Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits
13.6 mag. fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits
13.6 mag. fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits
All-image limiting magnitude estimate: 13.6 (SNR ) 10.9 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.mH11wkD4dq (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/Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.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_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits' -> 'wcs_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
WCS_IMAGE_NAME=wcs_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
WCS-calibrated image found: wcs_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
Checking if the catalog wcs_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits.cat corresponding to the image wcs_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits alredy exist and is non-empty...
Catalog wcs_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits.cat corresponding to the image wcs_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
WCS catalog name: wcs_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3206, passed=25547
Got 25547 stars (including 22312 good ones) from the SExtractor catalog wcs_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits.cat
util/solve_plate_with_UCAC5 got 25547 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 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 341.2187 through 0 to 19.8663, gap 19.8663 to 341.2187
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.4 to 67.4)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.47"
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 341.2185 through 0 to 19.8666, gap 19.8666 to 341.2185
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.4 to 67.4)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.47"
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits -region wcs_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.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.5HEwGiQNCz (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/Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.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_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits' -> 'wcs_Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits
WCS_IMAGE_NAME=wcs_Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits
WCS-calibrated image found: wcs_Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits
Checking if the catalog wcs_Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits.cat corresponding to the image wcs_Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits alredy exist and is non-empty...
Catalog wcs_Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits.cat corresponding to the image wcs_Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits
WCS catalog name: wcs_Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3160, passed=25477
Got 25477 stars (including 22297 good ones) from the SExtractor catalog wcs_Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits.cat
util/solve_plate_with_UCAC5 got 25477 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 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 341.2186 through 0 to 19.8660, gap 19.8660 to 341.2186
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.4 to 67.4)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.58"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.52"
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 341.2185 through 0 to 19.8672, gap 19.8672 to 341.2185
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.52"
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 977 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits -region wcs_Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.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.dBMxIPn7lC (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_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.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_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits
WCS_IMAGE_NAME=wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits
WCS-calibrated image found: wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits
Checking if the catalog wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits.cat corresponding to the image wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits.cat corresponding to the image wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits
WCS catalog name: wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=714, passed=8586
Got 8586 stars (including 7870 good ones) from the SExtractor catalog wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits.cat
util/solve_plate_with_UCAC5 got 8586 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.3'
Seting catalog search parameters based on the expected field of view 938.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013032 (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 0.010426 (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 340.6475 through 0 to 19.0531, gap 19.0531 to 340.6475
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.9 to 67.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 1.00"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 1.04"
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 340.6476 through 0 to 19.0569, gap 19.0569 to 340.6476
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.9 to 67.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 1.05"
Estimated accuracy of the plate solution: 1.13"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits -region wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.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.rwqDJrZXoC (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_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.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_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits
WCS_IMAGE_NAME=wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits
WCS-calibrated image found: wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits
Checking if the catalog wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits.cat corresponding to the image wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits.cat corresponding to the image wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits
WCS catalog name: wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits.cat
SExtractor catalog parsing summary: zero_flux=4, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=708, passed=8587
Got 8587 stars (including 7873 good ones) from the SExtractor catalog wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits.cat
util/solve_plate_with_UCAC5 got 8587 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.3'
Seting catalog search parameters based on the expected field of view 938.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013032 (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 0.010426 (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 340.6473 through 0 to 19.0526, gap 19.0526 to 340.6473
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.9 to 67.3)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 1.01"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 1.03"
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 340.6474 through 0 to 19.0565, gap 19.0565 to 340.6474
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.9 to 67.3)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 1.04"
Estimated accuracy of the plate solution: 1.14"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits -region wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.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_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/wcs_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits'
Saving fully-calibrated image wcs_Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/wcs_Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits'
Saving fully-calibrated image wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits'
Saving fully-calibrated image wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits'
Preparing the HTML report for the field Cas-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out31323.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32292.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out32729.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out09222.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10459.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 3s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31323_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 31323_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:11:02.85 +60:33:33.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.54, MAG_FAINT_SEARCH_LIMIT=11.52)GAIADR2_OUTPUT=# 1.164 2014060768131397376 347.76192149919 +60.55909415965 10.4665 9.7419 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.164#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32286_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 32286_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:36:00.36 +62:03:10.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32292_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 32292_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:48:14.12 +61:01:54.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.74, MAG_FAINT_SEARCH_LIMIT=11.72)GAIADR2_OUTPUT=# 1.572 2012585154812501376 357.05797580057 +61.03180192653 9.7857 8.2083 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.572#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32372_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 32372_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:24:57.51 +62:18:46.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32574_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 32574_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:41:26.42 +60:04:38.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32729_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 32729_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:13:34.48 +61:30:14.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.30, MAG_FAINT_SEARCH_LIMIT=12.28)GAIADR2_OUTPUT=# 0.764 2014960718396556160 348.39328831983 +61.50405602239 11.2145 10.2589 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.764#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03600_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 03600_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:46:53.86 +63:56:02.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09222_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 09222_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10459_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 10459_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 4s
Prepared the HTML report for the field Cas-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
00:20:13.72 +62:07:34.6
00:35:02.21 +61:18:56.2
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/Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits
SExtractor catalog cache: saved Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits.cat to cache
SExtractor catalog cache: saved Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
Creating symlink local_wcs_cache/wcs_Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits
Creating symlink local_wcs_cache/wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.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_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits exists and is non-empty
wcs_Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits exists and is non-empty
wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits exists and is non-empty
wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:00:01.853 +61:59:36.76
Second-epoch image center 23:59:59.312 +62:03:48.58
Angular distance between the image centers 0.07 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 00:00:01.853 +61:59:36.76
Second-epoch image center 23:59:56.815 +62:03:20.57
Angular distance between the image centers 0.06 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 23:59:59.312 +62:03:48.58
Second-epoch second image center 23:59:56.815 +62:03:20.57
Angular distance between the image centers 0.00918 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/Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits &> /tmp/tmp.v6dP86S16u
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits &> /tmp/tmp.twkAJQspqQ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits &> /tmp/tmp.UBWMG9KV0J
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits &> /tmp/tmp.ifyAuVydqu
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits
Calibrating the magnitude scale
Found non-empty wcs_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.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_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits and wcs_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.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_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits and wcs_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits.cat
Found non-empty wcs_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits and wcs_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits.cat
The reference image (wcs_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits) and catalog (wcs_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits.cat) found
'wcs_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits.cat' -> 'wcsmag.cat'
Read 170710 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 0.0001 to 360.0000 deg, Dec +55.3116 to +67.4209 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 360.0000 deg, Dec 55.3116 to 67.4209 deg
Loaded 133731 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): 10993 out of 16914 total matches.
Matched with Tycho-2 16914 out of 170710 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.762297
a=0.000000 b=1.000000 c=22.762297
From vast_summary.log: estimated ref. image limiting mag.: -7.62
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.14
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.14
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 199 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
2.3 pix Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits
2.9 pix fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits
2.9 pix fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits
Limiting magnitude estimates:
15.1 mag. Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
15.1 mag. Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits
13.7 mag. fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits
13.7 mag. fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits
All-image limiting magnitude estimate: 13.7 (SNR ) 13.1 (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.v6dP86S16u (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/Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.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_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits' -> 'wcs_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
WCS_IMAGE_NAME=wcs_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
WCS-calibrated image found: wcs_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
Checking if the catalog wcs_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits.cat corresponding to the image wcs_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits alredy exist and is non-empty...
Catalog wcs_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits.cat corresponding to the image wcs_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
WCS catalog name: wcs_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=35, blended=28495, passed=170675
Got 170675 stars (including 141953 good ones) from the SExtractor catalog wcs_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits.cat
util/solve_plate_with_UCAC5 got 170675 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 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 341.2187 through 0 to 20.1102, gap 20.1102 to 341.2187
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.51"
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 341.2185 through 0 to 20.1102, gap 20.1102 to 341.2185
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.51"
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits -region wcs_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.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.twkAJQspqQ (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/Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.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_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits' -> 'wcs_Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits
WCS_IMAGE_NAME=wcs_Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits
WCS-calibrated image found: wcs_Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits
Checking if the catalog wcs_Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits.cat corresponding to the image wcs_Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits alredy exist and is non-empty...
Catalog wcs_Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits.cat corresponding to the image wcs_Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits
WCS catalog name: wcs_Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=60, blended=28344, passed=170985
Got 170985 stars (including 142400 good ones) from the SExtractor catalog wcs_Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits.cat
util/solve_plate_with_UCAC5 got 170985 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 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 341.2186 through 0 to 20.0818, gap 20.0818 to 341.2186
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.53"
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 341.2184 through 0 to 20.0827, gap 20.0827 to 341.2184
Reading UCAC5 zone files...
Searching UCAC5 zones 726 to 789 (Dec 55.3 to 67.4)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.53"
Estimated accuracy of the plate solution: 0.56"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits -region wcs_Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.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.UBWMG9KV0J (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_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.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_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits
WCS_IMAGE_NAME=wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits
WCS-calibrated image found: wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits
Checking if the catalog wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits.cat corresponding to the image wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits.cat corresponding to the image wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits
WCS catalog name: wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=4501, passed=51599
Got 51599 stars (including 47067 good ones) from the SExtractor catalog wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits.cat
util/solve_plate_with_UCAC5 got 51599 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.3'
Seting catalog search parameters based on the expected field of view 938.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013032 (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 0.010426 (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 340.2534 through 0 to 19.2792, gap 19.2792 to 340.2534
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.8 to 67.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.96"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.92"
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 340.2535 through 0 to 19.2821, gap 19.2821 to 340.2535
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.8 to 67.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.93"
Estimated accuracy of the plate solution: 1.02"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits -region wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.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.ifyAuVydqu (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_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.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_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits
WCS_IMAGE_NAME=wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits
WCS-calibrated image found: wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits
Checking if the catalog wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits.cat corresponding to the image wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits alredy exist and is non-empty...
Catalog wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits.cat corresponding to the image wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits
WCS catalog name: wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=4689, passed=52028
Got 52028 stars (including 47311 good ones) from the SExtractor catalog wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits.cat
util/solve_plate_with_UCAC5 got 52028 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.3'
Seting catalog search parameters based on the expected field of view 938.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013032 (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 0.010426 (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 340.2554 through 0 to 19.2747, gap 19.2747 to 340.2554
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.8 to 67.3)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.95"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.92"
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 340.2552 through 0 to 19.2781, gap 19.2781 to 340.2552
Reading UCAC5 zone files...
Searching UCAC5 zones 729 to 788 (Dec 55.8 to 67.3)
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.92"
Estimated accuracy of the plate solution: 1.02"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits -region wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.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_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.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_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/wcs_Cas-02-Q2b1x1_2025-12-26_20-06-58_20.00sec_-15.00C_LIGHT_0063.fits
Saving fully-calibrated image wcs_Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.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_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/wcs_Cas-02-Q2b1x1_2025-12-26_20-07-54_20.00sec_-14.90C_LIGHT_0064.fits
Saving fully-calibrated image wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.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_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-02_20.00sec_-14.90C_LIGHT_0101.fits
Saving fully-calibrated image wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.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_2026-04-02_CI_Cas-02-Q2b1x1_054145_TTUQ2b1x1_13371_gF1nSCIx/wcs_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102.fits
Preparing the HTML report for the field Cas-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out181848.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out188600.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194879.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194884.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194887.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194890.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194891.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194893.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194894.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194896.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194898.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194901.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194915.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194916.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194923.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194926.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194928.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194933.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out197501.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198277.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198336.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198677.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198966.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out199130.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out199214.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out199335.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out199358.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out199573.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out199922.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out199954.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out199992.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200244.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200435.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200709.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out200834.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201025.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201076.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201258.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201558.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201576.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201693.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201825.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out201965.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202127.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out202190.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203062.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out38049.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out07777.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out100431.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out101029.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out10188.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out109784.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out11068.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out111340.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out111971.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out112079.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out113814.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115309.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116474.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out117708.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out119947.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out120115.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out120340.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out129203.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out130388.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133657.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136207.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138165.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138495.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out139685.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out145313.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out148112.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169818.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18826.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194903.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194907.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194927.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out194929.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out199257.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out201057.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out202510.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out203343.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22958.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23339.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24729.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25424.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31832.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35779.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35937.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37166.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38551.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41180.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43198.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45778.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out48326.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out49175.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51255.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53090.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53210.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out58687.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out59912.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out60128.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out61500.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out61673.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out63308.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out64855.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66455.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67279.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out71095.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out71228.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out71937.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77306.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78081.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82091.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82205.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out87578.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out90623.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out90694.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out91286.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out91927.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out92108.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out92225.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out92948.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out94769.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out94891.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out96299.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out98348.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 26s
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: 33s
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Considering the candidate 194879_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 194879_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:12:00.15 +63:16:51.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)
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Considering the candidate 194884_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 194884_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:50:40.93 +63:02:24.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 2.636 2016086755747753728 357.67075280749 +63.04092036662 12.7848 11.6470 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.636#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194887_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 194887_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:56:05.38 +65:43:46.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 5.871 525887031356689920 014.01851921161 +65.72933404043 11.9367 11.3980 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.871#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194890_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 194890_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:55:54.85 +65:19:50.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 1.707 524373416164485888 013.97950638833 +65.33105608480 11.9957 11.2902 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.707#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194891_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 194891_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:54:18.02 +63:45:25.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 3.966 523802975789106432 013.57355547069 +63.75612978221 12.0763 11.5429 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.966#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194893_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 194893_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:14:55.56 +61:19:54.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)
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Considering the candidate 194894_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 194894_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:24:35.66 +61:07:27.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)
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Considering the candidate 194896_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 194896_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:05:10.31 +57:55:09.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)GAIADR2_OUTPUT=# 3.867 422665635658165120 001.29347526610 +57.92020504116 12.2384 11.2453 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.867#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194898_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 194898_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:20:06.46 +63:22:46.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)
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Considering the candidate 194901_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 194901_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:17:23.90 +59:43:51.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 0.953 2010811470753650688 349.34930278549 +59.73125171075 12.4329 11.5273 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.953#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194903_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 194903_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
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Considering the candidate 194907_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 194907_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
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Considering the candidate 194915_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 194915_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:36:38.59 +58:37:21.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 4.431 2011025806799146112 354.16199881321 +58.62355819682 12.9640 12.0603 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.431#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194916_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 194916_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:45:56.52 +64:21:53.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)
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Considering the candidate 194917_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 194917_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:22:47.58 +64:28:50.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194923_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 194923_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:30:32.85 +58:59:42.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.76, MAG_FAINT_SEARCH_LIMIT=12.74)GAIADR2_OUTPUT=# 4.072 428043213891828480 007.63591910459 +58.99615725439 11.8177 11.4757 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.072#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 194926_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 194926_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:14:28.18 +60:51:50.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.93, MAG_FAINT_SEARCH_LIMIT=12.91)GAIADR2_OUTPUT=# 2.471 2014164908194686080 348.61621287714 +60.86430148926 12.2606 11.4554 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.471#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194927_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 194927_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194928_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 194928_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:02:20.46 +61:36:12.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.38, MAG_FAINT_SEARCH_LIMIT=12.36)GAIADR2_OUTPUT=# 0.460 429522190166156288 000.58508611573 +61.60349008593 11.1243 10.2083 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.460#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194929_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 194929_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 194931_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 194931_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:16:12.88 +60:59:38.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194933_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 194933_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:11:02.82 +60:33:32.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.64, MAG_FAINT_SEARCH_LIMIT=11.62)GAIADR2_OUTPUT=# 0.344 2014060768131397376 347.76192149919 +60.55909415965 10.4665 9.7419 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.344#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195584_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 195584_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:48:43.23 +62:13:31.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196389_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 196389_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:20:07.15 +61:57:13.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196791_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 196791_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:33:16.13 +62:54:25.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196820_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 196820_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:16:55.70 +60:26:00.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196971_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 196971_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:24:56.09 +61:36:36.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197112_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 197112_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:46:49.55 +58:40:33.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197341_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 197341_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:37:40.07 +58:50:46.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197358_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 197358_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:48:42.18 +62:11:04.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 197501_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 197501_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:19:56.80 +59:38:33.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197779_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 197779_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:24:38.54 +61:48:16.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 197800_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 197800_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:50:38.06 +64:12:38.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197812_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 197812_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:15:26.80 +57:27:08.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197850_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 197850_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:01:30.00 +60:19:21.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197938_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 197938_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:24:24.38 +61:38:16.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198031_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 198031_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:19:15.48 +65:08:08.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198059_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 198059_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:23:31.67 +63:19:20.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198277_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 198277_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:25:42.95 +60:48:44.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 4.125 2015381346013231488 351.43034390509 +60.81132477749 12.6651 12.1560 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.125#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198336_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 198336_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:21:32.04 +60:22:12.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 0.796 2013856190252769152 350.38313568210 +60.37021142379 10.5223 8.9797 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.796#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198470_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 198470_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:21:25.20 +59:13:55.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198493_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 198493_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:06:05.10 +61:04:33.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198551_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 198551_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:46:13.46 +60:30:00.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198559_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 198559_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:48:11.87 +65:05:35.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198571_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 198571_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:08:34.24 +63:10:15.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198668_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 198668_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:20:27.60 +61:52:31.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198677_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 198677_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:43:43.72 +62:44:34.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 3.686 2016009308897494272 355.93157723250 +62.74195673976 12.4126 11.9211 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.686#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 198690_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 198690_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:48:31.19 +62:14:40.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198727_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 198727_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:25:10.06 +62:18:20.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198966_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 198966_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:27:56.61 +65:22:42.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 1.305 2209508580691650816 351.98604053382 +65.37893925752 12.4526 11.8156 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.305#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199130_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 199130_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:24:38.60 +61:37:16.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 0.882 2015664161020968704 351.16042335484 +61.62148186941 12.2918 11.7918 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.882#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199189_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 199189_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:36:58.72 +63:07:58.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 199214_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 199214_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:55:16.90 +58:06:31.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199257_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 199257_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199306_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 199306_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:43:37.49 +61:06:04.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 199335_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 199335_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:15:53.69 +60:58:40.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 2.907 429560024543426688 003.97293956793 +60.97717267559 12.1003 11.5376 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.907#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199358_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 199358_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:28:16.79 +60:02:33.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.49, MAG_FAINT_SEARCH_LIMIT=13.47)GAIADR2_OUTPUT=# 1.614 2012276123320399744 352.06951098848 +60.04236123442 12.3638 11.2840 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.614#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199501_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 199501_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:25:04.78 +61:35:54.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 199516_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 199516_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:59:28.11 +63:50:32.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199537_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 199537_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:33:31.36 +60:26:49.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 199573_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 199573_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:26:33.11 +61:55:00.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 1.494 2015677320807840768 351.63883648771 +61.91679552162 12.5171 11.4506 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.494#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199577_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 199577_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:45:17.95 +62:30:46.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199797_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 199797_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:27:19.29 +65:35:47.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199850_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 199850_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:46:44.45 +62:34:37.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199922_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 199922_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:41:03.26 +65:06:23.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199933_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 199933_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:45:30.16 +63:53:57.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199954_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 199954_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:14:09.89 +62:12:55.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 1.852 2015227345665275520 348.54058455058 +62.21581341908 12.5302 11.5949 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.852#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199992_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 199992_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:18:22.52 +60:17:30.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 3.047 2013845366934250624 349.59415065649 +60.29258167705 13.0321 12.1315 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.047#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200012_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 200012_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:24:23.74 +61:37:46.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200244_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 200244_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:11:48.81 +66:20:51.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 5.380 528186870384605568 002.95170465070 +66.34883586507 11.3427 9.8221 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.380#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200282_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 200282_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:32:33.47 +64:05:31.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200360_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 200360_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:38:41.86 +61:19:04.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200412_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 200412_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:28:12.67 +61:29:36.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 200435_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 200435_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:51:02.28 +62:24:18.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 0.904 2013039493636740736 357.75971644855 +62.40545242111 13.1243 12.7310 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.904#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200680_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 200680_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:09:07.98 +59:39:13.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 200709_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 200709_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:57:31.42 +61:02:54.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 2.685 2011881634860716800 359.38243427849 +61.04842681350 12.5657 12.1950 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.685#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200718_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 200718_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:22:20.59 +59:19:15.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 200805_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 200805_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:04:08.10 +62:18:24.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200834_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 200834_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:12:02.78 +63:00:04.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 3.195 2207487369083671680 348.01110491822 +63.00027833451 13.1588 12.5321 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.195#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200861_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 200861_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:20:10.20 +61:08:49.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 200908_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 200908_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:42:41.33 +61:39:23.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 200955_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 200955_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:22:19.58 +60:08:11.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 200969_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 200969_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:56:16.01 +64:59:34.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201001_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 201001_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:00:54.40 +62:10:06.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201008_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 201008_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:17:06.46 +63:33:52.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201025_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 201025_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:19:11.01 +65:10:13.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 5.358 528053314082165760 004.79405808560 +65.17180567670 12.5216 11.5632 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.358#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 201057_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 201057_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
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Considering the candidate 201076_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 201076_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:40:46.60 +64:03:50.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 3.876 2017126275269097472 355.19662568634 +64.06408796051 13.1589 12.6179 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.876#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 201089_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 201089_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:04:52.61 +61:20:34.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201111_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 201111_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:41:43.69 +65:51:10.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201230_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 201230_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:27:09.39 +65:38:32.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201258_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 201258_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:26:43.73 +64:36:22.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)
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Considering the candidate 201526_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 201526_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:57:58.85 +59:43:21.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201558_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 201558_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:04:02.25 +64:40:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 3.233 432135939768630272 001.00734743558 +64.68207179636 12.6562 11.4542 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.233#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 201576_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 201576_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:52:26.65 +61:52:11.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 4.148 2012765436054414464 358.11346913519 +61.86972764825 12.7797 12.1353 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.148#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 201614_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 201614_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:32:53.24 +59:02:46.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201635_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 201635_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:46:06.71 +62:00:12.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201643_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 201643_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:23:52.74 +62:50:10.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201693_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 201693_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:37:02.99 +57:58:13.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 1.227 1998967836436757632 354.26227582676 +57.97011766909 12.4217 11.3757 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.227#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 201825_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 201825_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:21:09.84 +62:02:01.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)
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Considering the candidate 201965_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 201965_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:52:01.94 +65:39:32.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 2.154 2017555840714303232 358.00798329387 +65.65951345761 12.7813 11.8010 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.154#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202014_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 202014_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:29:26.88 +60:49:51.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 202127_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 202127_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:23:49.41 +60:28:01.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 1.556 2013859969824055168 350.95618803588 +60.46737592697 13.2965 12.8484 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.556#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202155_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 202155_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:19:06.36 +60:19:13.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 202190_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 202190_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:09:55.11 +61:24:39.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 1.899 2014908903910639872 347.48072632660 +61.41096935579 13.1229 12.3707 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.899#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 202510_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 202510_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
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Considering the candidate 202777_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 202777_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:53:22.05 +64:23:45.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 202969_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 202969_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:12:07.04 +62:53:28.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 203062_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 203062_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:44:09.07 +62:44:27.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 2.928 2016008415544667136 356.03928456291 +62.74135690867 13.2836 12.7080 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.928#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203343_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 203343_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 203604_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 203604_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:58:38.00 +60:40:21.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 203840_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 203840_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:42:18.58 +61:28:14.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 18826_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 18826_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 38049_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 38049_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:51:13.67 +62:38:13.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 3.391 523622350948126976 012.80851351045 +62.63775249768 11.5518 10.0003 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.391#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 82205_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 82205_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
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Considering the candidate 78081_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 78081_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
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Considering the candidate 59912_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 59912_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
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Considering the candidate 23283_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 23283_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:07:34.79 +64:43:18.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22958_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 22958_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 87578_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 87578_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
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Considering the candidate 92225_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 92225_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
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Considering the candidate 90362_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 90362_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:41:26.29 +60:04:38.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 41180_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 41180_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
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Considering the candidate 91927_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 91927_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
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Considering the candidate 119947_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 119947_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
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Considering the candidate 109784_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 109784_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
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Considering the candidate 94769_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 94769_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 60128_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 60128_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
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Considering the candidate 91286_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 91286_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 90623_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 90623_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61500_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 61500_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 130388_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 130388_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111971_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 111971_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 112079_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 112079_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 63308_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 63308_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 138165_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 138165_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 90227_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 90227_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:43:49.50 +60:00:27.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53210_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 53210_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62873_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 62873_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:20:13.71 +62:07:34.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 129203_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 129203_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 67279_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 67279_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
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Considering the candidate 66455_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 66455_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35779_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 35779_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11068_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 11068_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71810_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 71810_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 23:36:00.41 +62:03:10.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 80292_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 80292_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:48:06.37 +60:20:18.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 139685_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 139685_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
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Considering the candidate 35937_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 35937_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
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Considering the candidate 49175_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 49175_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71228_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 71228_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
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Considering the candidate 90694_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 90694_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116474_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 116474_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133657_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 133657_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 169818_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 169818_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
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Considering the candidate 138495_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 138495_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 77306_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 77306_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101029_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 101029_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 148112_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 148112_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 120115_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 120115_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52924_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 52924_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:12:26.05 +62:46:45.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 24729_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 24729_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 117708_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 117708_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 120340_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 120340_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10188_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 10188_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 135878_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 135878_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:31:42.76 +57:54:12.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 102223_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 102223_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:04:36.28 +60:18:17.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 43198_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 43198_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53090_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 53090_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58687_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 58687_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 111340_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 111340_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51255_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 51255_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136207_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 136207_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 98348_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 98348_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 64855_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 64855_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07777_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 07777_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 113814_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 113814_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 143077_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 143077_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:33:46.73 +58:15:40.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 96299_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 96299_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 145313_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 145313_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 115309_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 115309_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 48326_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 48326_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
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Considering the candidate 31832_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 31832_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61673_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 61673_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25424_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 25424_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
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Considering the candidate 71095_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 71095_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23339_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 23339_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22496_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 22496_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:46:53.77 +63:56:02.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82091_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 82091_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 94891_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 94891_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 45778_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 45778_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
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Considering the candidate 92948_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 92948_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
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Considering the candidate 37166_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 37166_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71937_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 71937_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 92108_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 92108_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
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Considering the candidate 181848_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 181848_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:23:56.89 +64:58:32.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 2.941 527287774812808064 005.98588746800 +64.97632156539 12.4218 10.9965 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.941#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 69913_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 69913_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:35:02.23 +61:18:56.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 38551_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 38551_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 188600_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
The candidate 188600_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102 did not pass the final checks
**** FOUND 00:32:25.23 +60:34:14.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 3.162 428611931978401024 008.10682973602 +60.57095886828 12.0615 10.4455 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.162#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100431_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
Preparing report for the candidate 100431_fd_Cas-02-Q2b1x1_2026-04-02_05-40-55_20.00sec_-15.00C_LIGHT_0102
make_report_in_HTML.sh Phase 2 (HTML assembly): 5s
make_report_in_HTML.sh TOTAL: 64s
Prepared the HTML report for the field Cas-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
00:20:13.72 +62:07:34.6
00:35:02.21 +61:18:56.2
00:34:42.32 +65:40:07.0
00:30:30.39 +59:50:50.4
00:04:40.43 +60:22:00.6
00:22:51.88 +65:40:24.5
00:31:19.62 +59:18:28.1
00:27:56.89 +65:26:12.0
23:43:06.20 +60:02:47.5
00:28:33.50 +59:15:27.4
00:27:28.62 +59:19:49.1
23:59:38.66 +59:45:29.6
23:54:45.03 +59:42:30.4
23:53:22.02 +59:38:43.4
23:44:25.45 +59:40:08.4
00:18:46.99 +59:05:05.1
23:57:58.44 +59:25:09.8
23:50:34.84 +59:27:31.0
23:56:17.94 +58:01:20.2
23:47:21.51 +58:13:17.1
00:24:11.86 +57:57:09.9
00:26:14.81 +58:05:38.3
23:54:36.76 +58:43:43.1
23:48:23.86 +58:50:27.9
23:47:12.55 +58:54:15.5
00:32:54.27 +58:24:23.1
00:15:13.34 +59:00:24.9
23:57:21.49 +58:25:05.1
00:34:25.82 +64:32:50.4
00:29:19.95 +60:02:41.7
00:57:01.27 +65:41:58.3
00:56:30.28 +65:09:58.8
00:57:01.45 +65:37:03.3
23:24:21.41 +61:36:20.7
23:46:05.16 +62:40:58.5
00:15:07.55 +66:20:31.6
00:52:22.45 +65:13:14.3
00:22:55.50 +64:31:43.0
00:39:01.97 +64:04:15.0
00:50:25.09 +63:36:02.9
00:52:21.15 +63:28:56.7
00:49:16.80 +63:10:03.4
00:10:53.44 +63:51:21.1
00:05:32.74 +63:52:38.5
00:51:25.01 +62:55:13.4
00:21:50.88 +63:25:59.9
00:52:02.98 +62:24:45.3
00:47:23.28 +62:28:01.4
23:58:43.98 +63:21:10.6
23:39:58.98 +63:20:52.6
00:48:32.67 +62:04:22.0
23:55:46.74 +63:04:26.3
00:12:18.99 +62:44:56.2
00:40:44.39 +62:05:03.5
00:34:30.84 +61:56:40.9
23:48:02.00 +62:37:47.5
00:48:55.20 +61:24:40.1
00:41:24.03 +61:33:20.4
00:39:02.29 +61:37:11.9
00:41:49.42 +61:28:42.8
23:39:27.28 +62:23:44.6
00:37:01.48 +61:25:08.5
23:57:22.05 +62:10:57.8
00:21:58.09 +61:32:43.9
00:35:25.34 +61:14:41.2
00:07:05.48 +61:48:53.5
00:39:38.72 +60:46:05.8
00:45:33.47 +60:31:45.7
00:46:50.29 +60:17:46.1
00:35:52.83 +60:37:12.8
23:46:09.44 +61:12:19.7
00:04:10.80 +60:55:22.0
00:28:08.17 +60:29:29.8
00:40:05.18 +60:01:37.1
00:04:06.97 +60:48:51.1
23:52:39.24 +60:56:06.3
23:48:14.14 +61:01:54.1
23:25:17.67 +60:57:31.8
00:08:21.87 +60:36:43.0
00:26:06.08 +60:15:13.6
00:27:09.45 +60:10:36.0
23:37:02.31 +60:42:00.8
########### Completed Cas-02-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
00:20:13.72 +62:07:34.6
00:35:02.21 +61:18:56.2
00:29:19.95 +60:02:41.7
00:57:01.27 +65:41:58.3
00:56:30.28 +65:09:58.8
00:57:01.45 +65:37:03.3
23:24:21.41 +61:36:20.7
23:46:05.16 +62:40:58.5
00:15:07.55 +66:20:31.6
00:52:22.45 +65:13:14.3
00:34:25.82 +64:32:50.4
00:35:52.83 +60:37:12.8
00:45:33.47 +60:31:45.7
23:48:02.00 +62:37:47.5
00:22:55.50 +64:31:43.0
23:46:09.44 +61:12:19.7
23:48:14.14 +61:01:54.1
00:52:02.98 +62:24:45.3
00:04:06.97 +60:48:51.1
00:18:46.99 +59:05:05.1
00:31:19.62 +59:18:28.1
00:08:21.87 +60:36:43.0
00:48:55.20 +61:24:40.1
00:40:05.18 +60:01:37.1
00:04:10.80 +60:55:22.0
00:41:24.03 +61:33:20.4
23:47:21.51 +58:13:17.1
00:28:33.50 +59:15:27.4
00:27:28.62 +59:19:49.1
00:41:49.42 +61:28:42.8
23:54:36.76 +58:43:43.1
00:40:44.39 +62:05:03.5
23:56:17.94 +58:01:20.2
23:57:22.05 +62:10:57.8
00:37:01.48 +61:25:08.5
00:10:53.44 +63:51:21.1
00:27:56.89 +65:26:12.0
23:47:12.55 +58:54:15.5
00:05:32.74 +63:52:38.5
00:48:32.67 +62:04:22.0
00:35:25.34 +61:14:41.2
00:28:08.17 +60:29:29.8
23:53:22.02 +59:38:43.4
00:24:11.86 +57:57:09.9
23:57:21.49 +58:25:05.1
23:48:23.86 +58:50:27.9
00:39:38.72 +60:46:05.8
00:04:40.43 +60:22:00.6
00:15:13.34 +59:00:24.9
23:57:58.44 +59:25:09.8
00:50:25.09 +63:36:02.9
23:44:25.45 +59:40:08.4
23:50:34.84 +59:27:31.0
00:22:51.88 +65:40:24.5
00:47:23.28 +62:28:01.4
00:12:18.99 +62:44:56.2
00:34:30.84 +61:56:40.9
23:43:06.20 +60:02:47.5
23:55:46.74 +63:04:26.3
00:26:14.81 +58:05:38.3
23:37:02.31 +60:42:00.8
23:39:27.28 +62:23:44.6
00:34:42.32 +65:40:07.0
23:59:38.66 +59:45:29.6
00:27:09.45 +60:10:36.0
00:32:54.27 +58:24:23.1
23:54:45.03 +59:42:30.4
23:39:58.98 +63:20:52.6
00:49:16.80 +63:10:03.4
00:39:02.29 +61:37:11.9
00:52:21.15 +63:28:56.7
00:21:58.09 +61:32:43.9
00:39:01.97 +64:04:15.0
00:46:50.29 +60:17:46.1
00:26:06.08 +60:15:13.6
23:58:43.98 +63:21:10.6
23:25:17.67 +60:57:31.8
00:51:25.01 +62:55:13.4
00:07:05.48 +61:48:53.5
23:52:39.24 +60:56:06.3
00:21:50.88 +63:25:59.9
00:30:30.39 +59:50:50.4
###################################################################################
00:20:13.72 +62:07:34.6 -- not an asteroid (will add it to exclusion list)
00:35:02.21 +61:18:56.2 -- not an asteroid (will add it to exclusion list)
00:29:19.95 +60:02:41.7 -- not an asteroid (will add it to exclusion list)
00:57:01.27 +65:41:58.3 -- not an asteroid (will add it to exclusion list)
00:56:30.28 +65:09:58.8 -- not an asteroid (will add it to exclusion list)
00:57:01.45 +65:37:03.3 -- not an asteroid (will add it to exclusion list)
23:24:21.41 +61:36:20.7 -- not an asteroid (will add it to exclusion list)
23:46:05.16 +62:40:58.5 -- not an asteroid (will add it to exclusion list)
00:15:07.55 +66:20:31.6 -- not an asteroid (will add it to exclusion list)
00:52:22.45 +65:13:14.3 -- not an asteroid (will add it to exclusion list)
00:34:25.82 +64:32:50.4 -- not an asteroid (will add it to exclusion list)
00:35:52.83 +60:37:12.8 -- not an asteroid (will add it to exclusion list)
00:45:33.47 +60:31:45.7 -- not an asteroid (will add it to exclusion list)
23:48:02.00 +62:37:47.5 -- not an asteroid (will add it to exclusion list)
00:22:55.50 +64:31:43.0 -- not an asteroid (will add it to exclusion list)
23:46:09.44 +61:12:19.7 -- not an asteroid (will add it to exclusion list)
23:48:14.14 +61:01:54.1 -- not an asteroid (will add it to exclusion list)
00:52:02.98 +62:24:45.3 -- not an asteroid (will add it to exclusion list)
00:04:06.97 +60:48:51.1 -- not an asteroid (will add it to exclusion list)
00:18:46.99 +59:05:05.1 -- not an asteroid (will add it to exclusion list)
00:31:19.62 +59:18:28.1 -- not an asteroid (will add it to exclusion list)
00:08:21.87 +60:36:43.0 -- not an asteroid (will add it to exclusion list)
00:48:55.20 +61:24:40.1 -- not an asteroid (will add it to exclusion list)
00:40:05.18 +60:01:37.1 -- not an asteroid (will add it to exclusion list)
00:04:10.80 +60:55:22.0 -- not an asteroid (will add it to exclusion list)
00:41:24.03 +61:33:20.4 -- not an asteroid (will add it to exclusion list)
23:47:21.51 +58:13:17.1 -- not an asteroid (will add it to exclusion list)
00:28:33.50 +59:15:27.4 -- not an asteroid (will add it to exclusion list)
00:27:28.62 +59:19:49.1 -- not an asteroid (will add it to exclusion list)
00:41:49.42 +61:28:42.8 -- not an asteroid (will add it to exclusion list)
23:54:36.76 +58:43:43.1 -- not an asteroid (will add it to exclusion list)
00:40:44.39 +62:05:03.5 -- not an asteroid (will add it to exclusion list)
23:56:17.94 +58:01:20.2 -- not an asteroid (will add it to exclusion list)
23:57:22.05 +62:10:57.8 -- not an asteroid (will add it to exclusion list)
00:37:01.48 +61:25:08.5 -- not an asteroid (will add it to exclusion list)
00:10:53.44 +63:51:21.1 -- not an asteroid (will add it to exclusion list)
00:27:56.89 +65:26:12.0 -- not an asteroid (will add it to exclusion list)
23:47:12.55 +58:54:15.5 -- not an asteroid (will add it to exclusion list)
00:05:32.74 +63:52:38.5 -- not an asteroid (will add it to exclusion list)
00:48:32.67 +62:04:22.0 -- not an asteroid (will add it to exclusion list)
00:35:25.34 +61:14:41.2 -- not an asteroid (will add it to exclusion list)
00:28:08.17 +60:29:29.8 -- not an asteroid (will add it to exclusion list)
23:53:22.02 +59:38:43.4 -- not an asteroid (will add it to exclusion list)
00:24:11.86 +57:57:09.9 -- not an asteroid (will add it to exclusion list)
23:57:21.49 +58:25:05.1 -- not an asteroid (will add it to exclusion list)
23:48:23.86 +58:50:27.9 -- not an asteroid (will add it to exclusion list)
00:39:38.72 +60:46:05.8 -- not an asteroid (will add it to exclusion list)
00:04:40.43 +60:22:00.6 -- not an asteroid (will add it to exclusion list)
00:15:13.34 +59:00:24.9 -- not an asteroid (will add it to exclusion list)
23:57:58.44 +59:25:09.8 -- not an asteroid (will add it to exclusion list)
00:50:25.09 +63:36:02.9 -- not an asteroid (will add it to exclusion list)
23:44:25.45 +59:40:08.4 -- not an asteroid (will add it to exclusion list)
23:50:34.84 +59:27:31.0 -- not an asteroid (will add it to exclusion list)
00:22:51.88 +65:40:24.5 -- not an asteroid (will add it to exclusion list)
00:47:23.28 +62:28:01.4 -- not an asteroid (will add it to exclusion list)
00:12:18.99 +62:44:56.2 -- not an asteroid (will add it to exclusion list)
00:34:30.84 +61:56:40.9 -- not an asteroid (will add it to exclusion list)
23:43:06.20 +60:02:47.5 -- not an asteroid (will add it to exclusion list)
23:55:46.74 +63:04:26.3 -- not an asteroid (will add it to exclusion list)
00:26:14.81 +58:05:38.3 -- not an asteroid (will add it to exclusion list)
23:37:02.31 +60:42:00.8 -- not an asteroid (will add it to exclusion list)
23:39:27.28 +62:23:44.6 -- not an asteroid (will add it to exclusion list)
00:34:42.32 +65:40:07.0 -- not an asteroid (will add it to exclusion list)
23:59:38.66 +59:45:29.6 -- not an asteroid (will add it to exclusion list)
00:27:09.45 +60:10:36.0 -- not an asteroid (will add it to exclusion list)
00:32:54.27 +58:24:23.1 -- not an asteroid (will add it to exclusion list)
23:54:45.03 +59:42:30.4 -- not an asteroid (will add it to exclusion list)
23:39:58.98 +63:20:52.6 -- not an asteroid (will add it to exclusion list)
00:49:16.80 +63:10:03.4 -- not an asteroid (will add it to exclusion list)
00:39:02.29 +61:37:11.9 -- not an asteroid (will add it to exclusion list)
00:52:21.15 +63:28:56.7 -- not an asteroid (will add it to exclusion list)
00:21:58.09 +61:32:43.9 -- not an asteroid (will add it to exclusion list)
00:39:01.97 +64:04:15.0 -- not an asteroid (will add it to exclusion list)
00:46:50.29 +60:17:46.1 -- not an asteroid (will add it to exclusion list)
00:26:06.08 +60:15:13.6 -- not an asteroid (will add it to exclusion list)
23:58:43.98 +63:21:10.6 -- not an asteroid (will add it to exclusion list)
23:25:17.67 +60:57:31.8 -- not an asteroid (will add it to exclusion list)
00:51:25.01 +62:55:13.4 -- not an asteroid (will add it to exclusion list)
00:07:05.48 +61:48:53.5 -- not an asteroid (will add it to exclusion list)
23:52:39.24 +60:56:06.3 -- not an asteroid (will add it to exclusion list)
00:21:50.88 +63:25:59.9 -- not an asteroid (will add it to exclusion list)
00:30:30.39 +59:50:50.4 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
00:04:06.97 +60:48:51.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:04:10.80 +60:55:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:04:40.43 +60:22:00.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:05:32.74 +63:52:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:07:05.48 +61:48:53.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:08:21.87 +60:36:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:10:53.44 +63:51:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:12:18.99 +62:44:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:15:07.55 +66:20:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:15:13.34 +59:00:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:18:46.99 +59:05:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:20:13.72 +62:07:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:21:50.88 +63:25:59.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:21:58.09 +61:32:43.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:22:51.88 +65:40:24.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:22:55.50 +64:31:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:24:11.86 +57:57:09.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:06.08 +60:15:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
00:26:14.81 +58:05:38.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:09.45 +60:10:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:28.62 +59:19:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:27:56.89 +65:26:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:28:08.17 +60:29:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:28:33.50 +59:15:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:29:19.95 +60:02:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:30:30.39 +59:50:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:31:19.62 +59:18:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:32:54.27 +58:24:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:25.82 +64:32:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:30.84 +61:56:40.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:34:42.32 +65:40:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:35:02.21 +61:18:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:35:25.34 +61:14:41.2 -- does not seem to be a hot pixel (will add it to exclusion list)
00:35:52.83 +60:37:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:37:01.48 +61:25:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:39:01.97 +64:04:15.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:39:02.29 +61:37:11.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:39:38.72 +60:46:05.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:40:05.18 +60:01:37.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:40:44.39 +62:05:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
00:41:24.03 +61:33:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:41:49.42 +61:28:42.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:45:33.47 +60:31:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:46:50.29 +60:17:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:47:23.28 +62:28:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:48:32.67 +62:04:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
00:48:55.20 +61:24:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
00:49:16.80 +63:10:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:50:25.09 +63:36:02.9 -- does not seem to be a hot pixel (will add it to exclusion list)
00:51:25.01 +62:55:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
00:52:02.98 +62:24:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:52:21.15 +63:28:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
00:52:22.45 +65:13:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:56:30.28 +65:09:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
00:57:01.27 +65:41:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
00:57:01.45 +65:37:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:24:21.41 +61:36:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:25:17.67 +60:57:31.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:37:02.31 +60:42:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:39:27.28 +62:23:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:39:58.98 +63:20:52.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:43:06.20 +60:02:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:44:25.45 +59:40:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:46:05.16 +62:40:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:46:09.44 +61:12:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
23:47:12.55 +58:54:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:47:21.51 +58:13:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:48:02.00 +62:37:47.5 -- does not seem to be a hot pixel (will add it to exclusion list)
23:48:14.14 +61:01:54.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:48:23.86 +58:50:27.9 -- does not seem to be a hot pixel (will add it to exclusion list)
23:50:34.84 +59:27:31.0 -- does not seem to be a hot pixel (will add it to exclusion list)
23:52:39.24 +60:56:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:53:22.02 +59:38:43.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:54:36.76 +58:43:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:54:45.03 +59:42:30.4 -- does not seem to be a hot pixel (will add it to exclusion list)
23:55:46.74 +63:04:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
23:56:17.94 +58:01:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
23:57:21.49 +58:25:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
23:57:22.05 +62:10:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:57:58.44 +59:25:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
23:58:43.98 +63:21:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
23:59:38.66 +59:45:29.6 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
00:04:06.97 +60:48:51.1 -- a known variable star
00:04:10.80 +60:55:22.0 -- a known variable star
00:04:40.43 +60:22:00.6 -- a known variable star
00:05:32.74 +63:52:38.5 -- a known variable star
00:07:05.48 +61:48:53.5 -- a known variable star
00:08:21.87 +60:36:43.0 -- a known variable star
00:10:53.44 +63:51:21.1 -- a known variable star
00:12:18.99 +62:44:56.2 -- a known variable star
00:15:07.55 +66:20:31.6 -- a known variable star
00:15:13.34 +59:00:24.9 -- a known variable star
00:18:46.99 +59:05:05.1 -- a known variable star
00:20:13.72 +62:07:34.6 -- a known variable star
00:21:50.88 +63:25:59.9 -- a known variable star
00:21:58.09 +61:32:43.9 -- a known variable star
00:22:51.88 +65:40:24.5 -- a known variable star
00:22:55.50 +64:31:43.0 -- a known variable star
00:24:11.86 +57:57:09.9 -- a known variable star
00:26:06.08 +60:15:13.6 -- a known variable star
00:26:14.81 +58:05:38.3 -- a known variable star
00:27:09.45 +60:10:36.0 -- a known variable star
00:27:28.62 +59:19:49.1 -- a known variable star
00:27:56.89 +65:26:12.0 -- a known variable star
00:28:08.17 +60:29:29.8 -- a known variable star
00:28:33.50 +59:15:27.4 -- a known variable star
00:29:19.95 +60:02:41.7 -- not a known variable star
00:30:30.39 +59:50:50.4 -- a known variable star
00:31:19.62 +59:18:28.1 -- a known variable star
00:32:54.27 +58:24:23.1 -- a known variable star
00:34:25.82 +64:32:50.4 -- a known variable star
00:34:30.84 +61:56:40.9 -- a known variable star
00:34:42.32 +65:40:07.0 -- a known variable star
00:35:02.21 +61:18:56.2 -- a known variable star
00:35:25.34 +61:14:41.2 -- a known variable star
00:35:52.83 +60:37:12.8 -- a known variable star
00:37:01.48 +61:25:08.5 -- a known variable star
00:39:01.97 +64:04:15.0 -- a known variable star
00:39:02.29 +61:37:11.9 -- a known variable star
00:39:38.72 +60:46:05.8 -- a known variable star
00:40:05.18 +60:01:37.1 -- a known variable star
00:40:44.39 +62:05:03.5 -- a known variable star
00:41:24.03 +61:33:20.4 -- a known variable star
00:41:49.42 +61:28:42.8 -- a known variable star
00:45:33.47 +60:31:45.7 -- a known variable star
00:46:50.29 +60:17:46.1 -- a known variable star
00:47:23.28 +62:28:01.4 -- a known variable star
00:48:32.67 +62:04:22.0 -- a known variable star
00:48:55.20 +61:24:40.1 -- a known variable star
00:49:16.80 +63:10:03.4 -- a known variable star
00:50:25.09 +63:36:02.9 -- a known variable star
00:51:25.01 +62:55:13.4 -- a known variable star
00:52:02.98 +62:24:45.3 -- not a known variable star
00:52:21.15 +63:28:56.7 -- a known variable star
00:52:22.45 +65:13:14.3 -- a known variable star
00:56:30.28 +65:09:58.8 -- not a known variable star
00:57:01.27 +65:41:58.3 -- not a known variable star
00:57:01.45 +65:37:03.3 -- not a known variable star
23:24:21.41 +61:36:20.7 -- not a known variable star
23:25:17.67 +60:57:31.8 -- a known variable star
23:37:02.31 +60:42:00.8 -- a known variable star
23:39:27.28 +62:23:44.6 -- a known variable star
23:39:58.98 +63:20:52.6 -- a known variable star
23:43:06.20 +60:02:47.5 -- a known variable star
23:44:25.45 +59:40:08.4 -- a known variable star
23:46:05.16 +62:40:58.5 -- not a known variable star
23:46:09.44 +61:12:19.7 -- a known variable star
23:47:12.55 +58:54:15.5 -- a known variable star
23:47:21.51 +58:13:17.1 -- a known variable star
23:48:02.00 +62:37:47.5 -- a known variable star
23:48:14.14 +61:01:54.1 -- a known variable star
23:48:23.86 +58:50:27.9 -- a known variable star
23:50:34.84 +59:27:31.0 -- a known variable star
23:52:39.24 +60:56:06.3 -- a known variable star
23:53:22.02 +59:38:43.4 -- a known variable star
23:54:36.76 +58:43:43.1 -- a known variable star
23:54:45.03 +59:42:30.4 -- a known variable star
23:55:46.74 +63:04:26.3 -- a known variable star
23:56:17.94 +58:01:20.2 -- a known variable star
23:57:21.49 +58:25:05.1 -- a known variable star
23:57:22.05 +62:10:57.8 -- a known variable star
23:57:58.44 +59:25:09.8 -- a known variable star
23:58:43.98 +63:21:10.6 -- a known variable star
23:59:38.66 +59:45:29.6 -- a known variable star
Found 7 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
82 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 82 (excluding asteroids and hot pixels), 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)2461132.94458920 -observatory V36
23:05:39.65 -07:27:53.3 Mercury (0.4mag)
02:03:53.20 +12:09:57.7 Venus (-3.9mag)
23:39:10.43 -03:23:06.6 Mars (1.2mag)
07:07:29.83 +22:54:14.2 Jupiter (-2.2mag)
00:23:03.12 +00:10:22.7 Saturn (0.9mag)
03:45:01.26 +19:38:47.6 Uranus (5.8mag)
00:09:01.00 -00:26:56.7 Neptune (7.8mag)
20:32:59.50 -22:52:37.9 Pluto (14.5mag)
12:53:00.55 -09:58:58.5 Moon (-12.7mag)
-rw-r--r-- 1 apache apache 362 Apr 2 05:45 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461132.94458920:
07:07:37.49 +22:53:58.3 Io (5.7mag)
07:07:42.62 +22:53:48.9 Europa (5.8mag)
07:07:38.34 +22:53:50.3 Ganymede (5.3mag)
07:07:45.44 +22:53:34.8 Callisto (6.5mag)
07:11:19.47 +22:48:45.4 Himalia (15.3mag)
07:07:33.71 +22:54:05.2 Thebe (16.1mag)
07:11:11.60 +23:16:34.9 Elara (17.2mag)
07:05:27.44 +23:41:20.6 Pasiphae (17.3mag)
07:16:05.76 +22:50:40.8 Carme (18.4mag)
00:22:55.60 +00:10:47.5 Titan (8.8mag)
00:23:01.17 +00:10:29.4 Rhea (10.1mag)
00:23:12.24 +00:12:17.9 Iapetus (11.5mag)
00:22:53.62 +00:10:30.5 Hyperion (14.8mag)
00:24:49.89 +00:20:33.5 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 2 05:45 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461132.94458920:
14:22:25.57 -04:41:21.9 JWST
20:02:33.43 -00:06:27.7 Chandra
08:54:27.52 -50:28:45.4 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 2 05:45 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461132.94458920 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:44:47.88 -28:02:40.7 14.0mag P/2010 H2 (Vales)
04:57:46.79 -70:20:40.6 17.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:29:59.86 +31:21:19.5 17.1mag C/2017 K2 (PANSTARRS)
17:30:52.87 +08:54:52.6 17.6mag C/2021 G2 (ATLAS)
23:06:07.08 +28:44:53.5 17.0mag C/2022 E2 (ATLAS)
04:13:48.93 +25:39:21.7 15.9mag C/2022 N2 (PANSTARRS)
09:01:35.04 +31:49:56.5 16.1mag C/2022 QE78 (ATLAS)
08:29:48.69 -01:40:00.6 17.3mag C/2022 R6 (PANSTARRS)
18:56:02.07 +17:22:10.6 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:44:23.05 -11:42:34.3 17.6mag P/2023 B1 (PANSTARRS)
09:15:11.99 -14:08:44.1 17.5mag C/2023 F3 (ATLAS)
21:38:52.80 +62:11:28.4 17.4mag C/2023 H5 (Lemmon)
19:28:30.13 -03:34:43.1 14.3mag C/2023 R1 (PANSTARRS)
21:42:55.37 +84:09:24.2 17.8mag C/2023 X2 (Lemmon)
06:13:58.16 +63:37:24.8 17.0mag C/2024 A1 (ATLAS)
04:41:48.00 +12:48:02.2 10.1mag C/2024 E1 (Wierzchos)
16:27:02.46 +04:09:48.3 17.4mag C/2024 G6 (ATLAS)
20:16:01.82 +11:44:12.0 14.8mag C/2024 J3 (ATLAS)
03:14:36.55 -24:32:04.5 16.4mag C/2024 T5 (ATLAS)
05:05:51.45 +48:52:18.4 17.6mag C/2025 J1 (Borisov)
14:33:31.24 +33:21:53.6 14.7mag C/2025 L1 (ATLAS)
03:05:00.79 -24:13:27.2 17.7mag C/2025 Q3 (ATLAS)
22:45:44.45 +19:45:27.6 10.7mag C/2025 R3 (PANSTARRS)
13:00:00.34 +02:08:41.0 17.5mag C/2025 Y1 (ATLAS)
01:20:10.29 +02:44:58.2 8.3mag C/2026 A1 (MAPS)
23:19:16.83 +34:23:04.0 14.1mag C/2026 B2 (Sun-Gao)
18:16:27.23 -10:23:20.1 12.6mag 10P/Tempel
15:17:04.17 +04:23:37.1 12.8mag 24P/Schaumasse
11:07:05.10 -02:00:10.1 15.7mag 29P/Schwassmann-Wachmann
17:54:23.53 -10:08:49.1 17.6mag 40P/Vaisala
10:39:53.95 -05:18:23.6 16.6mag 43P/Wolf-Harrington
01:27:49.22 +15:08:21.2 17.1mag 47P/Ashbrook-Jackson
06:47:06.45 +39:50:59.0 17.1mag 63P/Wild
23:11:18.47 -13:07:43.1 15.7mag 65P/Gunn
03:28:16.78 +16:18:54.6 15.8mag 76P/West-Kohoutek-Ikemura
00:35:59.08 +05:32:11.3 14.5mag 78P/Gehrels
22:20:29.22 -13:20:56.1 14.5mag 88P/Howell
01:33:05.03 +16:52:42.3 15.1mag 93P/Lovas
04:30:28.20 +31:29:46.8 16.3mag 123P/West-Hartley
08:14:40.98 +44:36:59.8 16.2mag 124P/Mrkos
02:12:35.51 +12:49:20.0 16.4mag 128P/Shoemaker-Holt
02:21:09.50 +12:45:25.4 17.4mag 131P/Mueller
00:17:30.17 +08:07:29.4 11.6mag 141P/Machholz
00:27:40.52 -00:10:21.1 11.6mag 141P-A/Machholz
23:20:30.33 -03:33:58.9 14.5mag 141P-D/Machholz
00:56:08.13 +01:25:14.0 18.0mag 141P-I/Machholz
00:24:47.12 -08:15:09.6 15.3mag 162P/SidingSpring
10:32:22.38 +31:42:17.4 17.7mag 164P/Christensen
06:11:37.78 +24:35:58.8 17.8mag 198P/ODAS
15:14:59.91 -01:40:45.8 17.2mag 210P/Christensen
20:56:34.61 -14:43:11.6 17.3mag 218P/LINEAR
17:10:14.46 -15:28:48.6 16.2mag 235P/LINEAR
05:05:56.68 +33:28:35.5 16.5mag 240P/NEAT
07:32:52.87 -06:44:45.8 17.6mag 242P/Spahr
15:46:52.23 +06:02:03.0 17.6mag 391P/Kowalski
07:29:57.46 +21:16:36.5 17.6mag 450P/LONEOS
05:16:49.01 +45:50:10.7 17.4mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 2 05:45 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.70 -27:51:49.80 SN2026gvk 2026-03-30 15.48
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.90 -45:55:38.40 ASASSN-26bt 2026-03-19.05 16.24
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.89 -15:50:13.40 AT2026fdy 2026-03-10.5 16.39
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.33 -37:49:33.00 ASASSN-26bk 2026-03-2.06 13.58
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.29 +19:58:46.30 ASASSN-26be 2026-02-25.56 14.95
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
11:50:37.32 +55:21:13.70 SN 2026dix 2026-02-21.43 16.39
16:21:19.69 -63:47:29.40 ASASSN-26az 2026-02-21.03 17.02
02:45:30.93 -54:17:43.10 SN 2026cju 2026-02-21.04 17.54
01:58:40.68 +47:34:50.10 ASASSN-26av 2026-02-21.09 15.97
18:35:53.01 -42:31:38.90 ASASSN-26aw 2026-02-21.12 15.89
11:40:18.88 -39:45:09.20 ASASSN-26ax 2026-02-21.08 15.73
02:26:23.52 -51:42:29.80 ASASSN-26ay 2026-02-21.04 13.93
08:46:07.66 +01:17:43.90 ASASSN-26ba 2026-02-20.23 15.43
14:15:47.69 -48:05:16.40 SN2026dez 2026-02-19.19 15.93
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.22 -11:25:16.10 AT2026bzh 2026-02-12.16 17.22
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
06:26:33.34 -54:06:39.90 AT2026cih 2026-02-8.06 17.26
23:08:59.40 -88:59:11.60 SN 2026bsu 2026-02-8.03 16.02
01:04:14.94 -62:31:02.30 SN 2026azk 2026-02-8.04 16.41
08:44:55.41 +64:55:09.90 SN 2026anq 2026-02-7.16 17.62
12:37:42.99 +33:26:05.40 SN 2026bnm 2026-02-7.29 16.74
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
22:34:01.26 +39:53:32.8 TCP J22340126+3953328 2026-01-17.5738 16.79Cmag
00:42:52.36 +41:16:13.3 PNV J00425236+4116133 2026-01-18.5502 17.41Cmag
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
-rw-r--r-- 1 apache apache 187K Apr 2 05:45 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
11:05:24.021 -16:51:22.17 AT 2026hki 2026-03-24.34 20.4438
10:36:26.290 -12:44:30.80 AT 2026hkh 2026-03-13.86 18
09:03:36.117 -67:58:13.34 SN 2026hkg 2026-03-27.12 18.505
08:08:11.420 -04:49:30.53 AT 2026hkf 2026-03-14.22 21.0121
04:20:57.978 -04:44:24.49 AT 2026hke 2026-03-26.13 19.8012
08:08:20.226 -14:40:00.64 AT 2026hkd 2026-03-07.19 20.1897
07:59:24.647 +57:00:58.39 AT 2026hkc 2026-03-14.20 20.9477
13:58:50.252 -17:03:03.26 AT 2026hkb 2026-03-23.24 19.315
08:55:52.185 -18:24:10.01 AT 2026hka 2026-03-20.39 19.87
19:49:11.846 -17:41:20.03 AT 2026hjz 2026-03-24.76 19.09
17:23:18.071 +42:30:08.80 AT 2026hjy 2026-03-15.19 19.329
15:36:56.914 -04:11:42.38 AT 2026hjx 2026-03-25.78 20.01
16:12:19.428 -02:04:41.40 AT 2026hjw 2026-03-24.64 20.22
11:18:56.464 -28:36:26.32 AT 2026hjv 2026-03-21.92 19.08
13:33:46.392 +11:46:20.90 AT 2026hju 2026-03-20.24 18.89
11:08:39.309 -42:07:08.38 AT 2026hjt 2026-03-25.18 19.306
18:40:00.884 -46:00:21.86 AT 2026hjs 2026-03-22.37 19.141
10:49:28.071 -32:24:01.15 AT 2026hjr 2026-03-21.92 19.476
08:13:57.386 +50:00:46.26 AT 2026hjq 2026-03-08.96 20.035
18:55:05.624 -41:25:59.25 AT 2026hjp 2026-03-24.79 20.17
-rw-r--r-- 1 apache apache 29K Apr 2 05:45 tns_transients_list.txt
