This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1223 Cyg,2461132.8691,10.79,0.05,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
V1223 Cyg 20260402.3691 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!
Don'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 25359,2461132.8691,9.49,0.05,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 25359 20260402.3691 9.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DU Cyg,2461132.8691,10.14,0.05,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
DU Cyg 20260402.3691 10.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
KZ Cyg,2461132.8691,9.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
KZ Cyg 20260402.3691 9.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2101579+402635,2461132.8691,10.34,0.05,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
NSVS J2101579+402635 20260402.3691 10.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
DR Cyg,2461132.8691,8.66,0.05,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
DR Cyg 20260402.3691 8.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J312.1986+36.4062,2461132.8691,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J312.1986+36.4062 20260402.3691 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1968500304814195456,2461132.8691,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1968500304814195456 20260402.3691 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSV 25471,2461132.8691,11.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 25471 20260402.3691 11.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don'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
V0529 Cyg,2461132.8691,11.55,0.05,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
V0529 Cyg 20260402.3691 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!
Don'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 1871723864011610368,2461132.8691,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1871723864011610368 20260402.3691 12.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2057825007406686208,2461132.8691,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2057825007406686208 20260402.3691 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2045170+342928,2461132.8691,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2045170+342928 20260402.3691 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don'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 25495,2461132.8691,10.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 25495 20260402.3691 10.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don'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 J205558.63+401754.9,2461132.8691,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J205558.63+401754.9 20260402.3691 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J211459.78+412810.8,2461132.8691,11.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J211459.78+412810.8 20260402.3691 11.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don'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 J210458.72+370801.7,2461132.8691,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J210458.72+370801.7 20260402.3691 12.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don'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 J2107187+404002,2461132.8691,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2107187+404002 20260402.3691 12.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J205833.05+403807.4,2461132.8691,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J205833.05+403807.4 20260402.3691 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J205958.88+391527.0,2461132.8691,11.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J205958.88+391527.0 20260402.3691 11.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don'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 J2101410+363658,2461132.8691,11.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2101410+363658 20260402.3691 11.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don'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 J205809.00+384807.0,2461132.8691,12.70,0.05,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
ZTF J205809.00+384807.0 20260402.3691 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 5892081,2461132.8691,10.64,0.05,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 5892081 20260402.3691 10.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 5878053,2461132.8691,12.06,0.05,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
NSVS 5878053 20260402.3691 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2041452+335323,2461132.8691,11.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2041452+335323 20260402.3691 11.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don'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
V3060 Cyg,2461132.8691,11.90,0.05,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
V3060 Cyg 20260402.3691 11.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2021473+360328,2461132.8691,12.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2021473+360328 20260402.3691 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don'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 J204742.15+340532.4,2461132.8691,11.69,0.05,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
ASASSN-V J204742.15+340532.4 20260402.3691 11.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1850 Cyg,2461132.8691,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1850 Cyg 20260402.3691 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don'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
V1489 Cyg,2461132.8691,13.11,0.05,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
V1489 Cyg 20260402.3691 13.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V2482 Cyg,2461132.8691,12.31,0.05,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
V2482 Cyg 20260402.3691 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!
Don'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 1868498343574788864,2461132.8691,12.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1868498343574788864 20260402.3691 12.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don'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
V1889 Cyg,2461132.8691,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1889 Cyg 20260402.3691 11.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don'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 8520852,2461132.8691,12.77,0.05,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
NSVS 8520852 20260402.3691 12.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1868598953191713408,2461132.8691,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1868598953191713408 20260402.3691 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J211246.49+402648.8,2461132.8691,11.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J211246.49+402648.8 20260402.3691 11.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don'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 J210353.37+380609.0,2461132.8691,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J210353.37+380609.0 20260402.3691 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J318.2525+36.8038,2461132.8691,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J318.2525+36.8038 20260402.3691 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don'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 5877962,2461132.8691,12.69,0.05,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
NSVS 5877962 20260402.3691 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J205741.92+352703.2,2461132.8691,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J205741.92+352703.2 20260402.3691 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0471 Cyg,2461132.8691,9.23,0.05,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
V0471 Cyg 20260402.3691 9.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J203931.01+343428.9,2461132.8691,12.87,0.05,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
ZTF J203931.01+343428.9 20260402.3691 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!
Don'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 J2047154+405912,2461132.8691,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2047154+405912 20260402.3691 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don'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
Mis V1017,2461132.8691,11.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Mis V1017 20260402.3691 11.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J210555.60+410916.7,2461132.8691,12.23,0.05,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
ASASSN-V J210555.60+410916.7 20260402.3691 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!
Don'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 J210939.70+413900.1,2461132.8691,12.35,0.05,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
ASASSN-V J210939.70+413900.1 20260402.3691 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!
Don'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 8515531,2461132.8691,11.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 8515531 20260402.3691 11.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don'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
V1886 Cyg,2461132.8691,10.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1886 Cyg 20260402.3691 10.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don'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 J211136.61+385242.4,2461132.8691,12.12,0.05,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
ASASSN-V J211136.61+385242.4 20260402.3691 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J203003.60+360605.8,2461132.8691,11.89,0.05,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 J203003.60+360605.8 20260402.3691 11.89CV 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!
Don'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 J203956.58+395526.8,2461132.8691,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J203956.58+395526.8 20260402.3691 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don'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 J205256.71+360455.4,2461132.8691,12.12,0.05,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
ASASSN-V J205256.71+360455.4 20260402.3691 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J204935.56+340734.0,2461132.8691,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J204935.56+340734.0 20260402.3691 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don'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 J210522.36+340026.7,2461132.8691,8.89,0.05,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
ASASSN-V J210522.36+340026.7 20260402.3691 8.89CV 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!
Don'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 J205658.67+344653.1,2461132.8691,12.59,0.05,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
ASASSN-V J205658.67+344653.1 20260402.3691 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1975 Cyg,2461132.8691,10.97,0.05,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
V1975 Cyg 20260402.3691 10.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1871 Cyg,2461132.8691,10.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1871 Cyg 20260402.3691 10.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J304.5162+37.7295,2461132.8691,12.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J304.5162+37.7295 20260402.3691 12.95CV 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!
Don'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 J210513.31+391324.5,2461132.8691,12.65,0.05,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 J210513.31+391324.5 20260402.3691 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J205334.25+404332.5,2461132.8691,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J205334.25+404332.5 20260402.3691 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2102100+373337,2461132.8691,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2102100+373337 20260402.3691 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461132.8691,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260402.3691 12.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don'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
V2481 Cyg,2461132.8691,9.65,0.05,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
V2481 Cyg 20260402.3691 9.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J205909.04+375255.1,2461132.8691,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J205909.04+375255.1 20260402.3691 11.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don'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 J205755.80+362440.9,2461132.8691,12.43,0.05,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
ASASSN-V J205755.80+362440.9 20260402.3691 12.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2106022+345000,2461132.8691,10.23,0.05,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
NSVS J2106022+345000 20260402.3691 10.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2053178+355418,2461132.8691,11.34,0.05,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
NSVS J2053178+355418 20260402.3691 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!
Don'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 25519,2461132.8691,10.80,0.05,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
NSV 25519 20260402.3691 10.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J210304.80+391230.7,2461132.8691,10.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J210304.80+391230.7 20260402.3691 10.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1840 Cyg,2461132.8691,12.66,0.05,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
V1840 Cyg 20260402.3691 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0528 Cyg,2461132.8691,11.02,0.05,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
V0528 Cyg 20260402.3691 11.02CV 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!
Don'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 8515293,2461132.8691,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 8515293 20260402.3691 12.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J205140.78+372906.0,2461132.8691,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J205140.78+372906.0 20260402.3691 12.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2105437+402558,2461132.8691,12.63,0.05,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
NSVS J2105437+402558 20260402.3691 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: 2461036.54686618 27.12.2025 01:07:19.238 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
First image: 2461036.54686618 27.12.2025 01:07:19.238 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
Last image: 2461132.86952034 02.04.2026 08:51:56.557 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 16
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.09
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: 6 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): 25052
Objects passed selection criteria: 24915
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 17019.5
Average stars matched: 15993.2 (93.9702 %)
Memory usage VmPeak: 128520 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 04:17:15 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: 2461036.54686618 27.12.2025 01:07:19.238 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
First image: 2461036.54686618 27.12.2025 01:07:19.238 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
Last image: 2461132.86952034 02.04.2026 08:51:56.557 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 247
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.74
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: 50 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): 171325
Objects passed selection criteria: 170764
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 117887
Average stars matched: 110062 (93.3621 %)
Memory usage VmPeak: 1927916 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 04:21:18 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/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits
SExtractor catalog cache: saved Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits.cat to cache
SExtractor catalog cache: saved Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.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/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.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: 2461132.86869672
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits exists and is non-empty
Saving wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits to local_wcs_cache/
'wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits' -> 'local_wcs_cache/wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits'
wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits exists and is non-empty
Saving wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits to local_wcs_cache/
'wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits' -> 'local_wcs_cache/wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits'
wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits exists and is non-empty
Saving wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits to local_wcs_cache/
'wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits' -> 'local_wcs_cache/wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits'
wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits exists and is non-empty
Saving wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits to local_wcs_cache/
'wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits' -> 'local_wcs_cache/wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.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 20:43:39.342 +38:00:09.97
Second-epoch image center 20:44:06.409 +37:59:51.19
Angular distance between the image centers 0.09 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 20:43:39.342 +38:00:09.97
Second-epoch image center 20:44:04.077 +38:00:28.46
Angular distance between the image centers 0.08 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 20:44:06.409 +37:59:51.19
Second-epoch second image center 20:44:04.077 +38:00:28.46
Angular distance between the image centers 0.01288 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/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits &> /tmp/tmp.pJxqNUmb2z
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits &> /tmp/tmp.h3Bs7qgwdi
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits &> /tmp/tmp.mb4m8TewEo
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits &> /tmp/tmp.fSi3GA5pTx
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.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_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits and wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.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_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits and wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits.cat
Found non-empty wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits and wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits.cat
The reference image (wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits) and catalog (wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits.cat) found
'wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits.cat' -> 'wcsmag.cat'
Read 30368 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 300.4603 to 321.7876 deg, Dec +32.1387 to +43.3386 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 300.4603 to 321.7876 deg, Dec 32.1387 to 43.3386 deg
Loaded 29500 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): 18486 out of 20549 total matches.
Matched with Tycho-2 20549 out of 30368 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.925229
a=0.000000 b=1.000000 c=22.925229
From vast_summary.log: estimated ref. image limiting mag.: -8.09
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.84
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.84
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 15 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.4 pix Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
2.4 pix Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits
3.0 pix fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits
2.9 pix fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits
Limiting magnitude estimates:
14.8 mag. Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
14.8 mag. Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits
13.6 mag. fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits
13.6 mag. fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.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.pJxqNUmb2z (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/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.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_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits' -> 'wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
WCS_IMAGE_NAME=wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
WCS-calibrated image found: wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
Checking if the catalog wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits.cat corresponding to the image wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits alredy exist and is non-empty...
Catalog wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits.cat corresponding to the image wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
WCS catalog name: wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3799, passed=30368
Got 30368 stars (including 26521 good ones) from the SExtractor catalog wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits.cat
util/solve_plate_with_UCAC5 got 30368 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.1 to 43.3)
Done reading UCAC5 zone files...
Matched 950 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: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.55"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.1 to 43.3)
Done reading UCAC5 zone files...
Matched 950 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.55"
Estimated accuracy of the plate solution: 0.57"
Excluding outliers - 945 stars left (next iteration limit 1040)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits -region wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.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.h3Bs7qgwdi (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/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.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_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits' -> 'wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits
WCS_IMAGE_NAME=wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits
WCS-calibrated image found: wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits
Checking if the catalog wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits.cat corresponding to the image wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits alredy exist and is non-empty...
Catalog wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits.cat corresponding to the image wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits
WCS catalog name: wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3780, passed=30367
Got 30367 stars (including 26553 good ones) from the SExtractor catalog wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits.cat
util/solve_plate_with_UCAC5 got 30367 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.1 to 43.3)
Done reading UCAC5 zone files...
Matched 953 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: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.54"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.1 to 43.3)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.54"
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 949 stars left (next iteration limit 1043)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits -region wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.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.mb4m8TewEo (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_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.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_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits
WCS-calibrated image found: wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits
Checking if the catalog wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits.cat corresponding to the image wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits.cat corresponding to the image wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.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_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits
WCS catalog name: wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=884, passed=10721
Got 10721 stars (including 9832 good ones) from the SExtractor catalog wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits.cat
util/solve_plate_with_UCAC5 got 10721 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010430 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 925 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: 0.94"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.97"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 925 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.98"
Estimated accuracy of the plate solution: 1.14"
Excluding outliers - 914 stars left (next iteration limit 1008)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits -region wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.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.fSi3GA5pTx (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_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.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_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits
WCS-calibrated image found: wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits
Checking if the catalog wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits.cat corresponding to the image wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits.cat corresponding to the image wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.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_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits
WCS catalog name: wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=931, passed=10821
Got 10821 stars (including 9878 good ones) from the SExtractor catalog wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits.cat
util/solve_plate_with_UCAC5 got 10821 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010430 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 925 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: 0.98"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.95"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 926 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.96"
Estimated accuracy of the plate solution: 1.11"
Excluding outliers - 917 stars left (next iteration limit 1009)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits -region wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.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_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits'
Saving fully-calibrated image wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits'
Saving fully-calibrated image wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits'
Saving fully-calibrated image wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits'
Preparing the HTML report for the field Cyg-06-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out18536.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out50065.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52069.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53560.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out05189.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out06079.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13156.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16280.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28657.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53296.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 4s
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Considering the candidate 52069_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 52069_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 21:04:16.72 +37:51:05.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.61, MAG_FAINT_SEARCH_LIMIT=10.59)GAIADR2_OUTPUT=# 4.280 1871887248876103680 316.07113251388 +37.85182772791 10.4930 8.7606 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.280#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 52090_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 52090_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:23:14.68 +40:45:19.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52837_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 52837_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:41:01.13 +39:05:44.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 53296_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 53296_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
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Considering the candidate 53469_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 53469_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:27:37.08 +35:33:18.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53560_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 53560_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:43:50.57 +34:28:50.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.94, MAG_FAINT_SEARCH_LIMIT=11.92)GAIADR2_OUTPUT=# 2.264 1870128992344684288 310.96042417085 +34.48016627940 9.7958 8.2778 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.264#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 50065_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 50065_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 21:03:04.56 +39:12:29.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.29, MAG_FAINT_SEARCH_LIMIT=11.27)GAIADR2_OUTPUT=# 3.222 1872224489712222976 315.77004430916 +39.20849364633 9.0371 7.5646 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.222#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18536_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 18536_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:56:13.52 +36:21:53.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.87, MAG_FAINT_SEARCH_LIMIT=11.85)GAIADR2_OUTPUT=# 0.911 1870027528041114368 314.05651234616 +36.36454214054 9.5481 7.9996 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.911#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 28657_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 28657_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
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Considering the candidate 23453_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 23453_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:46:37.76 +34:59:36.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 16280_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 16280_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
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Considering the candidate 05189_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 05189_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06079_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 06079_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07591_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 07591_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 21:10:19.02 +39:40:29.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 13156_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 13156_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 10s
Prepared the HTML report for the field Cyg-06-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 ####
20:27:23.12 +41:04:46.5
21:01:57.60 +40:26:31.9
20:43:41.12 +38:09:54.7
21:12:42.64 +36:44:18.2
20:50:14.92 +34:10:51.9
21:04:42.64 +41:12:39.8
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/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits
SExtractor catalog cache: saved Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits.cat to cache
SExtractor catalog cache: saved Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
Creating symlink local_wcs_cache/wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.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_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits exists and is non-empty
wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits exists and is non-empty
wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits exists and is non-empty
wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.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 20:43:39.342 +38:00:09.97
Second-epoch image center 20:44:06.409 +37:59:51.19
Angular distance between the image centers 0.09 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 20:43:39.342 +38:00:09.97
Second-epoch image center 20:44:04.077 +38:00:28.46
Angular distance between the image centers 0.08 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 20:44:06.409 +37:59:51.19
Second-epoch second image center 20:44:04.077 +38:00:28.46
Angular distance between the image centers 0.01288 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/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits &> /tmp/tmp.jMFyOwqzQi
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits &> /tmp/tmp.T18J8Epx7R
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits &> /tmp/tmp.4BKtW6TyeL
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits &> /tmp/tmp.li8GfCMSBJ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.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_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits and wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.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_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits and wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits.cat
Found non-empty wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits and wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits.cat
The reference image (wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits) and catalog (wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits.cat) found
'wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits.cat' -> 'wcsmag.cat'
Read 208031 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 300.4603 to 321.8236 deg, Dec +32.1226 to +43.3400 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 300.4603 to 321.8236 deg, Dec 32.1226 to 43.3400 deg
Loaded 29602 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): 14897 out of 22825 total matches.
Matched with Tycho-2 22825 out of 208031 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.749343
a=0.000000 b=1.000000 c=22.749343
From vast_summary.log: estimated ref. image limiting mag.: -7.74
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.01
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.01
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 210 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
2.2 pix Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits
2.8 pix fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits
2.8 pix fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits
Limiting magnitude estimates:
15.0 mag. Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
15.0 mag. Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits
13.6 mag. fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits
13.6 mag. fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits
All-image limiting magnitude estimate: 13.6 (SNR ) 13.0 (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.jMFyOwqzQi (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/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.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_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits' -> 'wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
WCS_IMAGE_NAME=wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
WCS-calibrated image found: wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
Checking if the catalog wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits.cat corresponding to the image wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits alredy exist and is non-empty...
Catalog wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits.cat corresponding to the image wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
WCS catalog name: wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=56, blended=36025, passed=207975
Got 207975 stars (including 171588 good ones) from the SExtractor catalog wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits.cat
util/solve_plate_with_UCAC5 got 207975 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.1 to 43.3)
Done reading UCAC5 zone files...
Matched 948 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: 0.57"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.1 to 43.3)
Done reading UCAC5 zone files...
Matched 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.57"
Estimated accuracy of the plate solution: 0.60"
Excluding outliers - 944 stars left (next iteration limit 1039)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits -region wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.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.T18J8Epx7R (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/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.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_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits' -> 'wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits
WCS_IMAGE_NAME=wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits
WCS-calibrated image found: wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits
Checking if the catalog wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits.cat corresponding to the image wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits alredy exist and is non-empty...
Catalog wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits.cat corresponding to the image wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits
WCS catalog name: wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=57, blended=35365, passed=205095
Got 205095 stars (including 169388 good ones) from the SExtractor catalog wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits.cat
util/solve_plate_with_UCAC5 got 205095 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.1 to 43.3)
Done reading UCAC5 zone files...
Matched 946 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: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.59"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.1 to 43.3)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.59"
Estimated accuracy of the plate solution: 0.63"
Excluding outliers - 941 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits -region wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.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.4BKtW6TyeL (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_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.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_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits
WCS-calibrated image found: wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits
Checking if the catalog wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits.cat corresponding to the image wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits.cat corresponding to the image wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.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_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits
WCS catalog name: wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=5758, passed=67013
Got 67013 stars (including 61186 good ones) from the SExtractor catalog wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits.cat
util/solve_plate_with_UCAC5 got 67013 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010430 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 920 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: 0.94"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 921 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.94"
Estimated accuracy of the plate solution: 1.12"
Excluding outliers - 910 stars left (next iteration limit 1005)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits -region wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.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.li8GfCMSBJ (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_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.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_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits
WCS-calibrated image found: wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits
Checking if the catalog wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits.cat corresponding to the image wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits.cat corresponding to the image wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.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_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits
WCS catalog name: wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=6017, passed=68762
Got 68762 stars (including 62670 good ones) from the SExtractor catalog wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits.cat
util/solve_plate_with_UCAC5 got 68762 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010430 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 924 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: 0.98"
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
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 925 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: 1.11"
Excluding outliers - 918 stars left (next iteration limit 1012)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits -region wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.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_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.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_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/wcs_Cyg-06-Q2b1x1_2025-12-26_19-07-19_20.00sec_-14.90C_LIGHT_0008.fits
Saving fully-calibrated image wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.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_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/wcs_Cyg-06-Q2b1x1_2025-12-26_19-08-13_20.00sec_-14.90C_LIGHT_0009.fits
Saving fully-calibrated image wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.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_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-50-45_20.00sec_-15.00C_LIGHT_0018.fits
Saving fully-calibrated image wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.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_Cyg-06-Q2b1x1_041458_TTUQ2b1x1_6755_sPxicJTR/wcs_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019.fits
Preparing the HTML report for the field Cyg-06-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out102944.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out219440.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out232407.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out232420.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out232421.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out232427.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out232429.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out232440.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out232443.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out232445.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out232452.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out232463.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out232465.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out236919.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out237313.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out237332.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out237403.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out23777.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out238059.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out238283.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out239025.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out239081.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out239478.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out240642.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out240666.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out241088.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out241416.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out242144.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out242226.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out242376.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out242518.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out242646.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out242681.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out242740.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out243538.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out243729.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out243859.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out244021.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out244164.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out244719.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out244838.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out244997.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out245018.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out245231.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out245717.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out245879.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out246050.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out247119.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out232435.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out100325.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103611.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104114.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107346.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out112053.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out117778.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out123463.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out126494.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out129768.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133274.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137069.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137082.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137681.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13820.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out142515.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out146592.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out152925.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16431.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out172598.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out172936.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out174517.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17575.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out178634.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out179548.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out181379.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out181910.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18481.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out185192.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out185739.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out185818.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out187168.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193355.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out196031.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out200921.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21557.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out232413.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out232433.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out235628.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out236879.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out241482.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out244713.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25523.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32328.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32470.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32516.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34394.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35030.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35630.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36536.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out42173.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46586.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51499.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out58002.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out59636.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out60176.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out62355.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65554.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68999.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out72603.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77147.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out78892.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82414.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out84024.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out86337.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out88862.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out89391.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95253.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out96928.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 32s
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: 30s
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Considering the candidate 232407_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 232407_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:17:57.85 +38:48:12.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 2.515 2061347842682280320 304.49070634050 +38.80403685290 13.1235 12.1921 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.515#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 232413_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 232413_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 232416_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 232416_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:56:07.69 +36:21:24.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 232420_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 232420_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:31:27.47 +38:33:54.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 1.753 2063913003289076480 307.86391481033 +38.56495692205 13.1573 12.6283 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.753#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 232421_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 232421_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:52:03.62 +37:31:47.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 3.256 1870942837114935808 313.01552212751 +37.53066822968 12.6629 12.1768 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.256#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 232422_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 232422_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:24:59.49 +33:39:48.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 232427_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 232427_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 21:07:33.29 +39:00:44.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.36, MAG_FAINT_SEARCH_LIMIT=13.34)
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Considering the candidate 232429_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 232429_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:16:46.84 +37:26:42.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 2.643 2060638692036150912 304.19443713466 +37.44463236424 12.7076 11.7330 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.643#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 232433_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 232433_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
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Considering the candidate 232435_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 232435_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 21:13:39.46 +38:58:13.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)
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Considering the candidate 232440_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 232440_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:54:19.34 +42:15:55.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 2.973 2065912396464956032 313.57953275947 +42.26575049468 12.4508 11.8659 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.973#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 232443_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 232443_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 21:16:11.20 +41:51:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 3.453 1968968456248943488 319.04573617731 +41.86377411104 11.4763 10.9751 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.453#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 232445_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 232445_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 21:04:46.51 +39:07:57.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 4.586 1872256130718127744 316.19539063690 +39.13232107179 12.1691 11.2764 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.586#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 232452_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 232452_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:23:49.07 +35:30:45.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 2.050 2057190108162866944 305.95375913585 +35.51253694123 12.1901 11.8224 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.050#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 232457_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 232457_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:27:01.75 +41:11:42.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 232461_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 232461_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:15:58.40 +37:57:53.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 232463_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 232463_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 21:13:09.50 +40:58:10.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.87, MAG_FAINT_SEARCH_LIMIT=11.85)GAIADR2_OUTPUT=# 3.571 1968543804244135936 318.28988181487 +40.97066036098 10.6026 9.6801 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.571#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 232465_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 232465_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:13:21.86 +35:03:39.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.12, MAG_FAINT_SEARCH_LIMIT=12.10)GAIADR2_OUTPUT=# 2.509 2055850834291009536 303.34187862575 +35.06124879401 11.1145 10.6797 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.509#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 233859_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 233859_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:41:01.17 +39:05:44.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234498_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 234498_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 21:04:42.65 +41:12:38.3 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 234529_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 234529_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:28:33.18 +39:08:57.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235628_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 235628_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 235808_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 235808_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:18:07.85 +37:11:25.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236117_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 236117_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:46:20.57 +34:01:00.4 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236879_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 236879_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 236919_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 236919_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:23:20.83 +40:46:45.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 1.836 2067567672561561984 305.83623034960 +40.77969861377 11.5957 10.6648 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.836#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237013_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 237013_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:17:42.41 +38:00:18.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 237092_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 237092_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:20:22.75 +39:22:59.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 237313_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 237313_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:17:02.16 +37:41:37.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 3.061 2060669340924492160 304.25824528536 +37.69435534623 11.8299 10.8838 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.061#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 237332_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 237332_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:46:59.88 +34:22:03.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.68, MAG_FAINT_SEARCH_LIMIT=12.66)GAIADR2_OUTPUT=# 1.396 1869341707664500224 311.74903067369 +34.36754567536 11.4229 10.6825 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.396#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 237388_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 237388_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:22:58.59 +40:46:12.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 237403_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 237403_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:18:03.42 +38:25:23.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 3.548 2061268639163669504 304.51330463037 +38.42395590397 12.3255 11.8941 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.548#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 238059_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 238059_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:23:53.30 +38:28:21.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 2.253 2061129933203706624 305.97129609183 +38.47277573861 11.2147 9.9494 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.253#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 238283_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 238283_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:28:43.66 +39:57:58.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 5.843 2067323860155172096 307.17989884620 +39.96685414058 12.3181 11.8428 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.843#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 238472_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 238472_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 21:14:57.20 +38:02:09.4 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 238629_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 238629_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:17:40.57 +38:00:59.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 239025_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 239025_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:51:33.32 +39:24:23.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 3.092 1872793624419599488 312.88793669081 +39.40689656986 11.6747 10.6130 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.092#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 239081_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 239081_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:21:34.86 +36:55:30.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.33, MAG_FAINT_SEARCH_LIMIT=13.31)GAIADR2_OUTPUT=# 1.129 2057938600702130432 305.39554544465 +36.92545635852 12.5703 12.0863 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.129#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 239478_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 239478_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:23:03.00 +40:46:26.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)GAIADR2_OUTPUT=# 5.375 2067570356920639104 305.76072533678 +40.77465039587 12.7075 12.0445 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.375#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 239628_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 239628_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:58:33.18 +41:22:36.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 239754_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 239754_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:13:49.28 +36:38:15.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 240037_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 240037_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:30:03.36 +38:32:26.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 240098_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 240098_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:25:42.08 +41:52:52.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 240201_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 240201_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 21:02:15.29 +39:29:18.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 240220_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 240220_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:17:15.37 +39:22:39.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 240434_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 240434_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 21:02:30.31 +39:30:02.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 240448_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 240448_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:36:36.29 +41:47:32.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 240480_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 240480_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:16:40.28 +37:41:21.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 240535_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 240535_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:14:14.84 +34:58:47.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 240642_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 240642_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:18:58.88 +39:01:56.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 3.436 2061358043216336256 304.74432774283 +39.03277090578 12.3218 11.2791 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.436#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 240666_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 240666_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:23:57.69 +38:30:35.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 2.370 2061130070642666880 305.98957624037 +38.50962628004 12.6184 11.9697 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.370#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 240759_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 240759_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:38:26.00 +42:04:48.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 240762_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 240762_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:18:23.48 +37:00:49.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 240779_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 240779_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:20:13.22 +39:19:30.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 240792_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 240792_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:14:01.45 +34:38:59.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 241088_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 241088_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:23:51.07 +38:28:17.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 2.819 2061129555246589824 305.96179501830 +38.47151798510 12.6016 11.9690 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.819#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 241290_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 241290_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 21:09:02.82 +38:44:26.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 241408_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 241408_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:19:09.89 +37:47:06.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 241416_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 241416_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 21:03:55.15 +34:04:14.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 1.059 1866361103432757248 315.97998617811 +34.07099596505 11.3613 9.8635 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.059#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 241482_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 241482_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 241519_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 241519_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:18:01.91 +37:11:03.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 241578_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 241578_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:17:05.26 +39:12:17.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 241715_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 241715_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:49:12.30 +35:35:27.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 241827_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 241827_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 21:00:42.20 +38:49:59.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 242087_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 242087_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:29:45.91 +41:38:33.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 242131_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 242131_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:20:57.78 +39:00:28.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 242144_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 242144_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:21:57.77 +40:44:14.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 2.925 2068314653274266368 305.48963610837 +40.73731095836 12.8776 12.1805 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.925#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 242157_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 242157_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:19:07.95 +39:12:49.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 242226_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 242226_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:57:30.51 +39:39:55.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.42, MAG_FAINT_SEARCH_LIMIT=13.40)GAIADR2_OUTPUT=# 3.126 1873219891327248512 314.37605043382 +39.66554156964 12.4182 11.9369 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.126#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 242286_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 242286_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:27:40.36 +42:03:11.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 242376_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 242376_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:17:30.91 +39:34:51.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 1.339 2062230956661052288 304.37922091257 +39.58066312203 12.8273 11.8710 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.339#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 242493_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 242493_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:21:42.51 +38:35:25.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 242518_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 242518_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:14:03.52 +37:54:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 3.595 2060903433824740736 303.51340347443 +37.91304933219 12.9788 12.4310 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.595#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 242616_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 242616_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:19:49.12 +37:09:21.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 242646_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 242646_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 21:03:12.32 +40:14:08.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 2.103 1873133304786912000 315.80062067190 +40.23593466331 12.2664 11.2771 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.103#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 242681_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 242681_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:13:38.52 +36:40:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 3.206 2060500634610233088 303.40996978620 +36.68308814909 12.7609 11.8070 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.206#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 242740_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 242740_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:16:55.64 +34:07:21.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 5.638 2055551389164929280 304.23010159127 +34.12206419186 12.5475 11.4767 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.638#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 242938_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 242938_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:25:51.40 +41:21:02.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 242959_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 242959_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:27:13.77 +34:20:23.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 243139_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 243139_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:21:07.99 +36:09:50.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 243446_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 243446_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:48:55.97 +39:46:49.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 243538_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 243538_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:28:28.20 +42:01:22.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 2.911 2068107945086244992 307.11654370718 +42.02338638866 12.9391 12.4560 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.911#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 243598_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 243598_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 21:07:57.85 +40:17:02.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 243719_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 243719_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:35:05.97 +34:49:50.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 243729_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 243729_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 21:11:40.08 +40:00:23.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 0.806 1968207624262460416 317.91675457133 +40.00646181997 12.0362 11.0447 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.806#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 243859_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 243859_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:24:38.38 +39:39:34.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 2.129 2067254350405094016 306.15993356392 +39.65907552052 13.2709 12.3846 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.129#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 243914_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 243914_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:15:04.56 +37:22:28.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 243980_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 243980_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:43:48.99 +35:25:38.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 243981_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 243981_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:36:41.50 +40:28:36.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 243992_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 243992_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:23:51.49 +37:28:54.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 244006_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 244006_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:54:30.51 +34:23:53.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244021_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 244021_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:19:10.95 +37:39:15.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 3.120 2061031866208979968 304.79460266042 +37.65453185048 12.4756 11.2716 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.120#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 244164_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 244164_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:21:57.83 +40:43:46.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 2.087 2068314657570896640 305.49024360942 +40.72948785549 13.3169 12.8527 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.087#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 244523_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 244523_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:37:42.44 +40:38:37.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244648_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 244648_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:42:12.19 +35:52:14.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244677_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 244677_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:35:33.62 +34:23:43.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244713_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 244713_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
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Considering the candidate 244719_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 244719_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:34:40.06 +34:53:45.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 3.351 1864349061573148288 308.66586786578 +34.89624457818 12.8665 12.3629 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.351#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 244838_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 244838_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:22:02.31 +38:35:25.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 3.303 2061179136350168064 305.50848644280 +38.59069509540 13.3786 12.8520 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.303#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 244997_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 244997_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:35:21.95 +35:12:08.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 4.061 2056606194471611520 308.84008081140 +35.20235231786 12.8496 10.7256 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.061#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 245018_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 245018_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:59:47.99 +34:20:08.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 1.682 1866602824191383168 314.94972146785 +34.33515903180 12.9518 11.0575 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.682#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 245099_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 245099_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:15:34.68 +39:44:39.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245231_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 245231_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:29:30.81 +34:12:41.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 3.326 2056091970929389440 307.37726373696 +34.21143242293 12.0742 10.6938 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.326#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 245262_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 245262_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:26:04.90 +38:52:01.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245715_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 245715_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:27:28.57 +38:25:04.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 245717_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 245717_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:42:35.47 +36:22:41.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 1.120 1870622943634010368 310.64740663614 +36.37814122419 12.6969 11.7599 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.120#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 245874_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 245874_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:28:31.76 +37:49:06.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 245879_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 245879_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:25:32.75 +40:01:18.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.17, MAG_FAINT_SEARCH_LIMIT=14.15)GAIADR2_OUTPUT=# 2.389 2067284140298564736 306.38560103332 +40.02184659941 13.2212 12.7368 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.389#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 246050_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 246050_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 21:04:14.82 +38:22:26.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 1.886 1872125705462432640 316.06221657140 +38.37434722551 12.7559 10.6262 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.886#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 246261_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 246261_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (24.6") between the two second-epoch detections
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Considering the candidate 246553_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 246553_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:33:58.40 +38:40:38.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246555_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 246555_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:48:35.99 +36:15:55.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 246629_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 246629_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:31:00.76 +36:54:14.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 246964_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 246964_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:27:29.28 +40:46:38.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 247053_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 247053_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:23:36.90 +37:28:14.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 247119_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 247119_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:44:01.09 +38:34:21.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 2.430 2063440934851222016 311.00416764941 +38.57330283637 13.7542 11.3135 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.430#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 185739_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 185739_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
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Considering the candidate 40808_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 40808_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 21:02:41.28 +40:14:04.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 86337_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 86337_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
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Considering the candidate 19400_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 19400_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 21:06:20.77 +41:35:48.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 42173_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 42173_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
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Considering the candidate 18481_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 18481_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
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Considering the candidate 149510_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 149510_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:27:37.01 +35:33:17.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103611_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 103611_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
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Considering the candidate 32470_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 32470_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
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Considering the candidate 35630_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 35630_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
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Considering the candidate 199050_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 199050_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:48:08.03 +35:01:07.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 59636_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 59636_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
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Considering the candidate 132183_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 132183_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:52:02.73 +36:07:58.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 117778_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 117778_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
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Considering the candidate 68999_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 68999_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
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Considering the candidate 78892_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 78892_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
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Considering the candidate 84024_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 84024_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
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Considering the candidate 102944_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 102944_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 21:13:48.72 +36:57:36.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.47, MAG_FAINT_SEARCH_LIMIT=12.45)GAIADR2_OUTPUT=# 1.905 1868603041990417664 318.45365959912 +36.96004735928 11.0194 10.1748 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.905#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 23222_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 23222_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 21:06:37.92 +41:17:10.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 181186_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 181186_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:50:14.98 +34:10:51.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 172936_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 172936_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
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Considering the candidate 200042_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 200042_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:46:37.81 +34:59:36.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65554_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 65554_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
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Considering the candidate 137069_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 137069_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
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Considering the candidate 178634_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 178634_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
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Considering the candidate 49182_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 49182_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 21:10:19.15 +39:40:30.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 142515_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 142515_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
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Considering the candidate 46586_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 46586_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
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Considering the candidate 23777_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 23777_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 21:09:00.29 +41:11:58.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 5.817 1969342565079852672 317.25294949878 +41.20047357908 13.2107 10.9411 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.817#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 71035_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 71035_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:59:24.56 +38:41:26.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 118361_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 118361_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:45:11.04 +36:48:41.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32516_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 32516_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
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Considering the candidate 112053_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 112053_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
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Considering the candidate 181379_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 181379_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
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Considering the candidate 193355_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 193355_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
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Considering the candidate 104114_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 104114_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
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Considering the candidate 89584_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 89584_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:43:41.11 +38:09:54.7 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 34394_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 34394_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
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Considering the candidate 89406_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 89406_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 21:03:03.59 +37:48:29.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82414_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 82414_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
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Considering the candidate 110702_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 110702_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 21:12:42.68 +36:44:17.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 107346_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 107346_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
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Considering the candidate 23453_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 23453_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 16431_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 16431_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
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Considering the candidate 146592_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 146592_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
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Considering the candidate 72603_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 72603_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
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Considering the candidate 187168_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 187168_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
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Considering the candidate 84266_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 84266_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:51:27.59 +38:13:59.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32328_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 32328_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
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Considering the candidate 77147_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 77147_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
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Considering the candidate 118564_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 118564_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:30:29.24 +36:51:52.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 38886_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 38886_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 21:01:57.65 +40:26:31.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 25523_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 25523_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17575_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 17575_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 185192_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 185192_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101438_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 101438_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:49:05.04 +37:27:28.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 126494_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 126494_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62355_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 62355_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137082_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 137082_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51499_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 51499_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 183224_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 183224_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:47:43.45 +34:19:04.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133274_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 133274_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 179548_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 179548_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 219440_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 219440_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:52:01.88 +37:35:43.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62530_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 62530_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 21:01:26.87 +39:03:32.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 181910_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 181910_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 196031_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 196031_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197574_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 197574_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:40:36.89 +35:01:41.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101123_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 101123_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 21:07:29.24 +37:10:44.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 185818_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 185818_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 152925_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 152925_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 96928_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 96928_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58002_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 58002_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62136_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 62136_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 21:12:30.67 +38:51:21.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35030_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 35030_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 199860_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 199860_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:36:11.85 +35:07:47.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 95253_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 95253_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129768_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 129768_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 88862_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 88862_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 89391_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 89391_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 123463_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 123463_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 200921_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 200921_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137681_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 137681_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 174907_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 174907_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:38:56.17 +33:59:58.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 66289_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 66289_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 21:01:14.15 +38:53:27.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21557_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 21557_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25322_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 25322_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 21:14:37.84 +40:57:40.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 60176_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 60176_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 172598_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 172598_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13820_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 13820_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32936_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
The candidate 32936_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019 did not pass the final checks
**** FOUND 20:27:23.14 +41:04:46.3 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 174517_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 174517_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 100325_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 100325_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36536_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
Preparing report for the candidate 36536_fd_Cyg-06-Q2b1x1_2026-04-02_03-51-56_20.00sec_-14.90C_LIGHT_0019
make_report_in_HTML.sh Phase 2 (HTML assembly): 4s
make_report_in_HTML.sh TOTAL: 66s
Prepared the HTML report for the field Cyg-06-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
20:27:23.12 +41:04:46.5
21:01:57.60 +40:26:31.9
20:43:41.12 +38:09:54.7
21:12:42.64 +36:44:18.2
20:50:14.92 +34:10:51.9
21:04:42.64 +41:12:39.8
20:51:40.55 +37:29:04.3
21:04:58.47 +37:08:03.0
21:14:08.49 +36:54:24.5
21:13:00.58 +36:47:45.1
21:12:03.21 +36:37:18.0
21:01:41.62 +36:36:58.9
20:57:55.81 +36:24:41.0
20:56:13.55 +36:21:52.5
20:45:56.94 +36:18:12.9
20:52:56.77 +36:04:54.9
20:21:48.36 +36:03:26.0
20:30:03.92 +36:06:06.3
20:53:17.81 +35:54:18.9
21:11:36.48 +41:51:36.2
20:47:56.66 +35:44:18.0
20:57:41.97 +35:27:01.9
20:51:40.64 +35:17:34.0
20:57:39.64 +41:56:58.9
20:45:46.75 +33:48:48.6
20:41:45.61 +33:53:24.6
20:33:50.71 +34:00:26.3
21:09:39.48 +41:38:57.2
20:47:42.28 +34:05:34.5
20:49:35.53 +34:07:36.4
20:57:10.27 +34:08:09.8
21:05:22.12 +34:00:28.7
21:14:59.36 +41:28:06.4
20:33:58.74 +34:30:35.5
20:45:16.94 +34:29:31.6
20:43:50.66 +34:28:50.4
20:39:31.23 +34:34:28.5
20:38:11.85 +34:50:56.4
20:56:58.73 +34:46:53.8
21:06:02.22 +34:50:02.3
21:12:47.46 +41:21:23.1
20:48:48.51 +36:24:21.0
21:11:01.93 +40:25:03.9
21:06:32.70 +37:32:49.9
21:12:59.33 +40:08:35.6
21:01:08.07 +37:56:52.5
20:27:26.00 +37:22:27.6
21:05:55.69 +41:09:11.1
20:47:15.63 +40:59:13.4
21:07:18.87 +40:40:11.1
21:07:39.35 +40:40:00.2
21:12:46.13 +40:26:46.1
20:53:34.32 +40:43:29.3
20:58:33.04 +40:38:04.3
21:05:43.78 +40:25:56.4
20:55:58.68 +40:17:50.6
20:46:25.76 +40:06:55.7
20:39:56.76 +39:55:24.1
21:05:13.33 +39:13:22.4
20:59:59.02 +39:15:25.1
21:03:04.68 +39:12:29.3
21:11:36.45 +38:52:42.1
20:39:36.79 +39:12:07.8
20:58:09.11 +38:48:06.3
21:07:07.51 +38:34:03.9
21:01:37.80 +38:23:16.3
21:12:48.03 +38:06:41.4
21:03:53.34 +38:06:07.1
20:59:35.62 +38:06:24.0
21:09:43.60 +37:49:31.6
21:04:16.76 +37:51:05.3
20:59:09.01 +37:52:53.9
21:02:09.93 +37:33:34.6
20:18:04.76 +37:44:15.7
########### Completed Cyg-06-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 ####
21:04:42.64 +41:12:39.8
20:50:14.92 +34:10:51.9
21:12:42.64 +36:44:18.2
20:27:23.12 +41:04:46.5
21:01:57.60 +40:26:31.9
20:43:41.12 +38:09:54.7
20:48:48.51 +36:24:21.0
21:11:01.93 +40:25:03.9
21:06:32.70 +37:32:49.9
21:12:59.33 +40:08:35.6
21:01:08.07 +37:56:52.5
20:27:26.00 +37:22:27.6
20:45:16.94 +34:29:31.6
21:09:43.60 +37:49:31.6
20:55:58.68 +40:17:50.6
21:14:59.36 +41:28:06.4
21:04:58.47 +37:08:03.0
21:07:18.87 +40:40:11.1
20:58:33.04 +40:38:04.3
20:59:59.02 +39:15:25.1
21:01:41.62 +36:36:58.9
20:58:09.11 +38:48:06.3
21:12:48.03 +38:06:41.4
20:59:35.62 +38:06:24.0
20:41:45.61 +33:53:24.6
20:39:36.79 +39:12:07.8
20:21:48.36 +36:03:26.0
20:47:42.28 +34:05:34.5
20:47:56.66 +35:44:18.0
20:46:25.76 +40:06:55.7
21:07:39.35 +40:40:00.2
21:12:03.21 +36:37:18.0
20:57:10.27 +34:08:09.8
20:38:11.85 +34:50:56.4
21:14:08.49 +36:54:24.5
21:12:46.13 +40:26:46.1
21:03:53.34 +38:06:07.1
21:13:00.58 +36:47:45.1
20:57:39.64 +41:56:58.9
20:57:41.97 +35:27:01.9
21:07:07.51 +38:34:03.9
20:39:31.23 +34:34:28.5
20:47:15.63 +40:59:13.4
21:01:37.80 +38:23:16.3
21:05:55.69 +41:09:11.1
21:09:39.48 +41:38:57.2
20:33:58.74 +34:30:35.5
20:56:13.55 +36:21:52.5
21:11:36.45 +38:52:42.1
20:30:03.92 +36:06:06.3
20:39:56.76 +39:55:24.1
20:52:56.77 +36:04:54.9
20:49:35.53 +34:07:36.4
21:05:22.12 +34:00:28.7
20:56:58.73 +34:46:53.8
20:43:50.66 +34:28:50.4
20:51:40.64 +35:17:34.0
20:18:04.76 +37:44:15.7
21:05:13.33 +39:13:22.4
20:53:34.32 +40:43:29.3
21:02:09.93 +37:33:34.6
20:45:56.94 +36:18:12.9
21:04:16.76 +37:51:05.3
20:59:09.01 +37:52:53.9
20:57:55.81 +36:24:41.0
21:06:02.22 +34:50:02.3
20:53:17.81 +35:54:18.9
21:12:47.46 +41:21:23.1
21:03:04.68 +39:12:29.3
20:45:46.75 +33:48:48.6
21:11:36.48 +41:51:36.2
20:33:50.71 +34:00:26.3
20:51:40.55 +37:29:04.3
21:05:43.78 +40:25:56.4
###################################################################################
21:04:42.64 +41:12:39.8 -- not an asteroid (will add it to exclusion list)
20:50:14.92 +34:10:51.9 -- not an asteroid (will add it to exclusion list)
21:12:42.64 +36:44:18.2 -- not an asteroid (will add it to exclusion list)
20:27:23.12 +41:04:46.5 -- not an asteroid (will add it to exclusion list)
21:01:57.60 +40:26:31.9 -- not an asteroid (will add it to exclusion list)
20:43:41.12 +38:09:54.7 -- not an asteroid (will add it to exclusion list)
20:48:48.51 +36:24:21.0 -- not an asteroid (will add it to exclusion list)
21:11:01.93 +40:25:03.9 -- not an asteroid (will add it to exclusion list)
21:06:32.70 +37:32:49.9 -- not an asteroid (will add it to exclusion list)
21:12:59.33 +40:08:35.6 -- not an asteroid (will add it to exclusion list)
21:01:08.07 +37:56:52.5 -- not an asteroid (will add it to exclusion list)
20:27:26.00 +37:22:27.6 -- not an asteroid (will add it to exclusion list)
20:45:16.94 +34:29:31.6 -- not an asteroid (will add it to exclusion list)
21:09:43.60 +37:49:31.6 -- not an asteroid (will add it to exclusion list)
20:55:58.68 +40:17:50.6 -- not an asteroid (will add it to exclusion list)
21:14:59.36 +41:28:06.4 -- not an asteroid (will add it to exclusion list)
21:04:58.47 +37:08:03.0 -- not an asteroid (will add it to exclusion list)
21:07:18.87 +40:40:11.1 -- not an asteroid (will add it to exclusion list)
20:58:33.04 +40:38:04.3 -- not an asteroid (will add it to exclusion list)
20:59:59.02 +39:15:25.1 -- not an asteroid (will add it to exclusion list)
21:01:41.62 +36:36:58.9 -- not an asteroid (will add it to exclusion list)
20:58:09.11 +38:48:06.3 -- not an asteroid (will add it to exclusion list)
21:12:48.03 +38:06:41.4 -- not an asteroid (will add it to exclusion list)
20:59:35.62 +38:06:24.0 -- not an asteroid (will add it to exclusion list)
20:41:45.61 +33:53:24.6 -- not an asteroid (will add it to exclusion list)
20:39:36.79 +39:12:07.8 -- not an asteroid (will add it to exclusion list)
20:21:48.36 +36:03:26.0 -- not an asteroid (will add it to exclusion list)
20:47:42.28 +34:05:34.5 -- not an asteroid (will add it to exclusion list)
20:47:56.66 +35:44:18.0 -- not an asteroid (will add it to exclusion list)
20:46:25.76 +40:06:55.7 -- not an asteroid (will add it to exclusion list)
21:07:39.35 +40:40:00.2 -- not an asteroid (will add it to exclusion list)
21:12:03.21 +36:37:18.0 -- not an asteroid (will add it to exclusion list)
20:57:10.27 +34:08:09.8 -- not an asteroid (will add it to exclusion list)
20:38:11.85 +34:50:56.4 -- not an asteroid (will add it to exclusion list)
21:14:08.49 +36:54:24.5 -- not an asteroid (will add it to exclusion list)
21:12:46.13 +40:26:46.1 -- not an asteroid (will add it to exclusion list)
21:03:53.34 +38:06:07.1 -- not an asteroid (will add it to exclusion list)
21:13:00.58 +36:47:45.1 -- not an asteroid (will add it to exclusion list)
20:57:39.64 +41:56:58.9 -- not an asteroid (will add it to exclusion list)
20:57:41.97 +35:27:01.9 -- not an asteroid (will add it to exclusion list)
21:07:07.51 +38:34:03.9 -- not an asteroid (will add it to exclusion list)
20:39:31.23 +34:34:28.5 -- not an asteroid (will add it to exclusion list)
20:47:15.63 +40:59:13.4 -- not an asteroid (will add it to exclusion list)
21:01:37.80 +38:23:16.3 -- not an asteroid (will add it to exclusion list)
21:05:55.69 +41:09:11.1 -- not an asteroid (will add it to exclusion list)
21:09:39.48 +41:38:57.2 -- not an asteroid (will add it to exclusion list)
20:33:58.74 +34:30:35.5 -- not an asteroid (will add it to exclusion list)
20:56:13.55 +36:21:52.5 -- not an asteroid (will add it to exclusion list)
21:11:36.45 +38:52:42.1 -- not an asteroid (will add it to exclusion list)
20:30:03.92 +36:06:06.3 -- not an asteroid (will add it to exclusion list)
20:39:56.76 +39:55:24.1 -- not an asteroid (will add it to exclusion list)
20:52:56.77 +36:04:54.9 -- not an asteroid (will add it to exclusion list)
20:49:35.53 +34:07:36.4 -- not an asteroid (will add it to exclusion list)
21:05:22.12 +34:00:28.7 -- not an asteroid (will add it to exclusion list)
20:56:58.73 +34:46:53.8 -- not an asteroid (will add it to exclusion list)
20:43:50.66 +34:28:50.4 -- not an asteroid (will add it to exclusion list)
20:51:40.64 +35:17:34.0 -- not an asteroid (will add it to exclusion list)
20:18:04.76 +37:44:15.7 -- not an asteroid (will add it to exclusion list)
21:05:13.33 +39:13:22.4 -- not an asteroid (will add it to exclusion list)
20:53:34.32 +40:43:29.3 -- not an asteroid (will add it to exclusion list)
21:02:09.93 +37:33:34.6 -- not an asteroid (will add it to exclusion list)
20:45:56.94 +36:18:12.9 -- not an asteroid (will add it to exclusion list)
21:04:16.76 +37:51:05.3 -- not an asteroid (will add it to exclusion list)
20:59:09.01 +37:52:53.9 -- not an asteroid (will add it to exclusion list)
20:57:55.81 +36:24:41.0 -- not an asteroid (will add it to exclusion list)
21:06:02.22 +34:50:02.3 -- not an asteroid (will add it to exclusion list)
20:53:17.81 +35:54:18.9 -- not an asteroid (will add it to exclusion list)
21:12:47.46 +41:21:23.1 -- not an asteroid (will add it to exclusion list)
21:03:04.68 +39:12:29.3 -- not an asteroid (will add it to exclusion list)
20:45:46.75 +33:48:48.6 -- not an asteroid (will add it to exclusion list)
21:11:36.48 +41:51:36.2 -- not an asteroid (will add it to exclusion list)
20:33:50.71 +34:00:26.3 -- not an asteroid (will add it to exclusion list)
20:51:40.55 +37:29:04.3 -- not an asteroid (will add it to exclusion list)
21:05:43.78 +40:25:56.4 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
20:18:04.76 +37:44:15.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:21:48.36 +36:03:26.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:27:23.12 +41:04:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:27:26.00 +37:22:27.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:30:03.92 +36:06:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:33:50.71 +34:00:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:33:58.74 +34:30:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:38:11.85 +34:50:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:39:31.23 +34:34:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:39:36.79 +39:12:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:39:56.76 +39:55:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:41:45.61 +33:53:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:43:41.12 +38:09:54.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:43:50.66 +34:28:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:45:16.94 +34:29:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:45:46.75 +33:48:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:45:56.94 +36:18:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:46:25.76 +40:06:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:47:15.63 +40:59:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:47:42.28 +34:05:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:47:56.66 +35:44:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:48:48.51 +36:24:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:49:35.53 +34:07:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:50:14.92 +34:10:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:51:40.55 +37:29:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:51:40.64 +35:17:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:52:56.77 +36:04:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:53:17.81 +35:54:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:53:34.32 +40:43:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:55:58.68 +40:17:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:13.55 +36:21:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:56:58.73 +34:46:53.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:10.27 +34:08:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:39.64 +41:56:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:41.97 +35:27:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:57:55.81 +36:24:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:09.11 +38:48:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:58:33.04 +40:38:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:59:09.01 +37:52:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:59:35.62 +38:06:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:59:59.02 +39:15:25.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:08.07 +37:56:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:37.80 +38:23:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:41.62 +36:36:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:01:57.60 +40:26:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:02:09.93 +37:33:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:03:04.68 +39:12:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:03:53.34 +38:06:07.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:04:16.76 +37:51:05.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:04:42.64 +41:12:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
21:04:58.47 +37:08:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:05:13.33 +39:13:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:05:22.12 +34:00:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
21:05:43.78 +40:25:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:05:55.69 +41:09:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:06:02.22 +34:50:02.3 -- does not seem to be a hot pixel (will add it to exclusion list)
21:06:32.70 +37:32:49.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:07:07.51 +38:34:03.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:07:18.87 +40:40:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:07:39.35 +40:40:00.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:09:39.48 +41:38:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:09:43.60 +37:49:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:11:01.93 +40:25:03.9 -- does not seem to be a hot pixel (will add it to exclusion list)
21:11:36.45 +38:52:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:11:36.48 +41:51:36.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:12:03.21 +36:37:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
21:12:42.64 +36:44:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
21:12:46.13 +40:26:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:12:47.46 +41:21:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:12:48.03 +38:06:41.4 -- does not seem to be a hot pixel (will add it to exclusion list)
21:12:59.33 +40:08:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
21:13:00.58 +36:47:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
21:14:08.49 +36:54:24.5 -- does not seem to be a hot pixel (will add it to exclusion list)
21:14:59.36 +41:28:06.4 -- 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)
20:18:04.76 +37:44:15.7 -- not a known variable star
20:21:48.36 +36:03:26.0 -- a known variable star
20:27:23.12 +41:04:46.5 -- a known variable star
20:27:26.00 +37:22:27.6 -- a known variable star
20:30:03.92 +36:06:06.3 -- a known variable star
20:33:50.71 +34:00:26.3 -- a known variable star
20:33:58.74 +34:30:35.5 -- a known variable star
20:38:11.85 +34:50:56.4 -- a known variable star
20:39:31.23 +34:34:28.5 -- a known variable star
20:39:36.79 +39:12:07.8 -- a known variable star
20:39:56.76 +39:55:24.1 -- a known variable star
20:41:45.61 +33:53:24.6 -- a known variable star
20:43:41.12 +38:09:54.7 -- a known variable star
20:43:50.66 +34:28:50.4 -- a known variable star
20:45:16.94 +34:29:31.6 -- a known variable star
20:45:46.75 +33:48:48.6 -- a known variable star
20:45:56.94 +36:18:12.9 -- a known variable star
20:46:25.76 +40:06:55.7 -- a known variable star
20:47:15.63 +40:59:13.4 -- a known variable star
20:47:42.28 +34:05:34.5 -- a known variable star
20:47:56.66 +35:44:18.0 -- a known variable star
20:48:48.51 +36:24:21.0 -- not a known variable star
20:49:35.53 +34:07:36.4 -- a known variable star
20:50:14.92 +34:10:51.9 -- a known variable star
20:51:40.55 +37:29:04.3 -- a known variable star
20:51:40.64 +35:17:34.0 -- a known variable star
20:52:56.77 +36:04:54.9 -- a known variable star
20:53:17.81 +35:54:18.9 -- a known variable star
20:53:34.32 +40:43:29.3 -- a known variable star
20:55:58.68 +40:17:50.6 -- a known variable star
20:56:13.55 +36:21:52.5 -- a known variable star
20:56:58.73 +34:46:53.8 -- a known variable star
20:57:10.27 +34:08:09.8 -- a known variable star
20:57:39.64 +41:56:58.9 -- a known variable star
20:57:41.97 +35:27:01.9 -- a known variable star
20:57:55.81 +36:24:41.0 -- a known variable star
20:58:09.11 +38:48:06.3 -- a known variable star
20:58:33.04 +40:38:04.3 -- a known variable star
20:59:09.01 +37:52:53.9 -- a known variable star
20:59:35.62 +38:06:24.0 -- a known variable star
20:59:59.02 +39:15:25.1 -- a known variable star
21:01:08.07 +37:56:52.5 -- not a known variable star
21:01:37.80 +38:23:16.3 -- a known variable star
21:01:41.62 +36:36:58.9 -- a known variable star
21:01:57.60 +40:26:31.9 -- a known variable star
21:02:09.93 +37:33:34.6 -- a known variable star
21:03:04.68 +39:12:29.3 -- a known variable star
21:03:53.34 +38:06:07.1 -- a known variable star
21:04:16.76 +37:51:05.3 -- a known variable star
21:04:42.64 +41:12:39.8 -- a known variable star
21:04:58.47 +37:08:03.0 -- a known variable star
21:05:13.33 +39:13:22.4 -- a known variable star
21:05:22.12 +34:00:28.7 -- a known variable star
21:05:43.78 +40:25:56.4 -- a known variable star
21:05:55.69 +41:09:11.1 -- a known variable star
21:06:02.22 +34:50:02.3 -- a known variable star
21:06:32.70 +37:32:49.9 -- a known variable star
21:07:07.51 +38:34:03.9 -- a known variable star
21:07:18.87 +40:40:11.1 -- a known variable star
21:07:39.35 +40:40:00.2 -- a known variable star
21:09:39.48 +41:38:57.2 -- a known variable star
21:09:43.60 +37:49:31.6 -- a known variable star
21:11:01.93 +40:25:03.9 -- not a known variable star
21:11:36.45 +38:52:42.1 -- a known variable star
21:11:36.48 +41:51:36.2 -- a known variable star
21:12:03.21 +36:37:18.0 -- a known variable star
21:12:42.64 +36:44:18.2 -- a known variable star
21:12:46.13 +40:26:46.1 -- a known variable star
21:12:47.46 +41:21:23.1 -- a known variable star
21:12:48.03 +38:06:41.4 -- a known variable star
21:12:59.33 +40:08:35.6 -- a known variable star
21:13:00.58 +36:47:45.1 -- not a known variable star
21:14:08.49 +36:54:24.5 -- not a known variable star
21:14:59.36 +41:28:06.4 -- a known variable star
Found 6 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
74 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 74 (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)2461132.86869672 -observatory V36
23:05:22.96 -07:28:53.7 Mercury (0.4mag)
02:03:31.77 +12:07:52.2 Venus (-3.9mag)
23:38:57.30 -03:24:32.0 Mars (1.2mag)
07:07:28.45 +22:54:16.4 Jupiter (-2.2mag)
00:23:01.02 +00:10:09.5 Saturn (0.9mag)
03:45:00.41 +19:38:44.9 Uranus (5.8mag)
00:09:00.37 -00:27:00.7 Neptune (7.8mag)
20:32:59.18 -22:52:38.1 Pluto (14.5mag)
12:50:42.05 -09:35:18.4 Moon (-12.7mag)
-rw-r--r-- 1 apache apache 362 Apr 2 04:17 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461132.86869672:
07:07:36.49 +22:54:00.5 Io (5.7mag)
07:07:40.80 +22:53:52.4 Europa (5.8mag)
07:07:38.20 +22:53:50.4 Ganymede (5.3mag)
07:07:44.99 +22:53:35.3 Callisto (6.5mag)
07:11:18.20 +22:48:50.1 Himalia (15.3mag)
07:07:32.57 +22:54:08.7 Thebe (16.1mag)
07:11:10.23 +23:16:38.4 Elara (17.2mag)
07:05:25.75 +23:41:25.2 Pasiphae (17.3mag)
07:16:04.45 +22:50:42.4 Carme (18.4mag)
00:22:53.69 +00:10:34.4 Titan (8.8mag)
00:22:58.75 +00:10:17.0 Rhea (10.1mag)
00:23:10.31 +00:12:05.0 Iapetus (11.5mag)
00:22:51.40 +00:10:17.8 Hyperion (14.8mag)
00:24:47.85 +00:20:20.7 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 2 04:17 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461132.86869672:
14:22:21.03 -04:36:55.1 JWST
19:44:38.83 +06:50:35.6 Chandra
08:32:16.92 -47:04:38.1 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 2 04:17 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461132.86869672 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:44:44.95 -28:02:26.7 14.0mag P/2010 H2 (Vales)
04:57:44.03 -70:20:55.2 17.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:29:59.19 +31:21:18.1 17.1mag C/2017 K2 (PANSTARRS)
17:30:52.74 +08:54:19.3 17.6mag C/2021 G2 (ATLAS)
23:06:05.52 +28:44:44.9 17.0mag C/2022 E2 (ATLAS)
04:13:43.84 +25:39:13.8 15.9mag C/2022 N2 (PANSTARRS)
09:01:34.80 +31:49:50.8 16.1mag C/2022 QE78 (ATLAS)
08:29:48.55 -01:40:32.7 17.2mag C/2022 R6 (PANSTARRS)
18:56:02.54 +17:21:46.7 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:44:24.08 -11:42:37.7 17.6mag P/2023 B1 (PANSTARRS)
09:15:14.99 -14:09:31.5 17.5mag C/2023 F3 (ATLAS)
21:38:47.04 +62:11:15.1 17.4mag C/2023 H5 (Lemmon)
19:28:32.50 -03:34:41.1 14.3mag C/2023 R1 (PANSTARRS)
21:42:54.84 +84:08:51.4 17.8mag C/2023 X2 (Lemmon)
06:13:57.66 +63:37:28.4 17.0mag C/2024 A1 (ATLAS)
04:41:36.28 +12:45:46.6 10.1mag C/2024 E1 (Wierzchos)
16:27:04.76 +04:09:03.7 17.4mag C/2024 G6 (ATLAS)
20:15:59.90 +11:43:03.7 14.8mag C/2024 J3 (ATLAS)
03:14:32.72 -24:32:49.6 16.4mag C/2024 T5 (ATLAS)
05:05:47.99 +48:53:35.8 17.6mag C/2025 J1 (Borisov)
14:33:48.46 +33:16:43.0 14.7mag C/2025 L1 (ATLAS)
03:04:54.30 -24:12:49.5 17.7mag C/2025 Q3 (ATLAS)
22:45:36.69 +19:45:16.3 10.7mag C/2025 R3 (PANSTARRS)
13:00:02.32 +02:08:22.8 17.5mag C/2025 Y1 (ATLAS)
01:20:45.92 +02:40:18.6 8.4mag C/2026 A1 (MAPS)
23:19:02.59 +34:21:58.2 14.1mag C/2026 B2 (Sun-Gao)
18:16:18.44 -10:23:31.7 12.6mag 10P/Tempel
15:17:09.29 +04:23:56.5 12.8mag 24P/Schaumasse
11:07:06.77 -02:00:20.4 15.7mag 29P/Schwassmann-Wachmann
17:54:20.50 -10:09:00.1 17.6mag 40P/Vaisala
10:39:55.39 -05:18:50.4 16.6mag 43P/Wolf-Harrington
01:27:42.21 +15:07:32.9 17.1mag 47P/Ashbrook-Jackson
06:46:58.95 +39:51:55.7 17.1mag 63P/Wild
23:11:12.32 -13:08:17.7 15.7mag 65P/Gunn
03:28:05.37 +16:17:09.3 15.8mag 76P/West-Kohoutek-Ikemura
00:35:49.22 +05:31:16.5 14.5mag 78P/Gehrels
22:20:14.38 -13:22:13.5 14.5mag 88P/Howell
01:32:52.79 +16:51:23.5 15.1mag 93P/Lovas
04:30:20.39 +31:29:29.8 16.3mag 123P/West-Hartley
08:14:37.24 +44:39:07.2 16.2mag 124P/Mrkos
02:12:28.65 +12:48:48.1 16.4mag 128P/Shoemaker-Holt
02:21:00.65 +12:44:48.6 17.4mag 131P/Mueller
00:17:08.05 +08:05:39.7 11.6mag 141P/Machholz
00:27:18.57 -00:12:00.0 11.6mag 141P-A/Machholz
23:20:11.22 -03:35:20.3 14.5mag 141P-D/Machholz
00:55:45.31 +01:23:29.2 18.0mag 141P-I/Machholz
00:24:34.47 -08:17:22.3 15.3mag 162P/SidingSpring
10:32:24.32 +31:42:31.1 17.7mag 164P/Christensen
06:11:29.48 +24:36:04.2 17.8mag 198P/ODAS
15:15:07.59 -01:41:21.8 17.2mag 210P/Christensen
20:56:19.33 -14:44:15.9 17.3mag 218P/LINEAR
17:10:11.46 -15:29:17.3 16.2mag 235P/LINEAR
05:05:47.29 +33:28:07.0 16.5mag 240P/NEAT
07:32:51.35 -06:45:19.9 17.6mag 242P/Spahr
15:46:53.31 +06:01:42.7 17.6mag 391P/Kowalski
07:29:56.37 +21:16:33.9 17.6mag 450P/LONEOS
05:16:42.82 +45:50:27.6 17.4mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 2 04:17 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
-rw-r--r-- 1 apache apache 5.8K Apr 2 04:17 asassn_transients_list.txt
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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 04:17 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
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
14:10:06.186 +10:00:51.42 AT 2026hjo 2026-03-24.40 20.2791
08:47:29.260 +16:55:56.97 AT 2026hjn 2026-03-20.25 20.8588
08:53:19.672 -26:00:27.80 AT 2026hjm 2026-03-26.19 19.4129
-rw-r--r-- 1 apache apache 29K Apr 2 04:17 tns_transients_list.txt
