This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX
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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSV 25018,2461139.8086,10.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 25018 20260409.3086 10.90CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-10970,2461139.8086,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-10970 20260409.3086 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J286.4262+37.0592,2461139.8086,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J286.4262+37.0592 20260409.3086 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J301.5076+37.2500,2461139.8086,11.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J301.5076+37.2500 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-00200,2461139.8086,10.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-00200 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J200332.82+355653.3,2461139.8086,10.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J200332.82+355653.3 20260409.3086 10.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1295 Cyg,2461139.8086,10.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1295 Cyg 20260409.3086 10.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J192457.98+361257.4,2461139.8086,10.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J192457.98+361257.4 20260409.3086 10.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1673 Cyg,2461139.8086,10.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1673 Cyg 20260409.3086 10.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0451 Cyg,2461139.8086,9.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0451 Cyg 20260409.3086 9.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-01723,2461139.8086,11.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-01723 20260409.3086 11.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1297 Cyg,2461139.8086,10.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1297 Cyg 20260409.3086 10.89CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
OQ Cyg,2461139.8086,11.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
OQ Cyg 20260409.3086 11.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J301.3779+37.6564,2461139.8086,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J301.3779+37.6564 20260409.3086 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2073435319441286656,2461139.8086,13.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 2073435319441286656 20260409.3086 13.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J303.6381+39.5422,2461139.8086,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J303.6381+39.5422 20260409.3086 13.32CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.8086,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.3086 13.19CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J296.9468+36.3212,2461139.8086,13.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J296.9468+36.3212 20260409.3086 13.27CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2045661488244626560,2461139.8086,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 2045661488244626560 20260409.3086 13.19CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J296.0566+40.4540,2461139.8086,13.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J296.0566+40.4540 20260409.3086 13.40CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2073142991101417472,2461139.8086,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 2073142991101417472 20260409.3086 13.38CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J296.0097+36.1557,2461139.8086,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J296.0097+36.1557 20260409.3086 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J300.6225+37.1042,2461139.8086,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J300.6225+37.1042 20260409.3086 13.09CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J295.0920+41.8638,2461139.8086,13.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J295.0920+41.8638 20260409.3086 13.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J287.5573+34.3756,2461139.8086,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J287.5573+34.3756 20260409.3086 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.1298+38.8377,2461139.8086,13.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J299.1298+38.8377 20260409.3086 13.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J301.4301+40.0717,2461139.8086,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J301.4301+40.0717 20260409.3086 13.09CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J296.1106+35.8460,2461139.8086,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J296.1106+35.8460 20260409.3086 12.99CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J303.9642+39.1089,2461139.8086,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J303.9642+39.1089 20260409.3086 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J298.9813+36.0503,2461139.8086,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J298.9813+36.0503 20260409.3086 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2048136591994231168,2461139.8086,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 2048136591994231168 20260409.3086 12.99CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J294.2914+37.9055,2461139.8086,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J294.2914+37.9055 20260409.3086 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2071734929040770560,2461139.8086,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 2071734929040770560 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.8086,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.3086 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J195414.00+375236.5,2461139.8086,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J195414.00+375236.5 20260409.3086 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J194215.92+335944.4,2461139.8086,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J194215.92+335944.4 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J200604.64+390915.2,2461139.8086,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J200604.64+390915.2 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J297.2417+33.1963,2461139.8086,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J297.2417+33.1963 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2059177063137623936,2461139.8086,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 2059177063137623936 20260409.3086 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J200353.95+395244.3,2461139.8086,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J200353.95+395244.3 20260409.3086 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2060282828242418176,2461139.8086,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 2060282828242418176 20260409.3086 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J298.0373+38.9736,2461139.8086,12.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J298.0373+38.9736 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J304.3712+38.4802,2461139.8086,12.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J304.3712+38.4802 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
MGAB-V926,2461139.8086,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
MGAB-V926 20260409.3086 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2060507231681529088,2461139.8086,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 2060507231681529088 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J302.2914+33.4555,2461139.8086,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J302.2914+33.4555 20260409.3086 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-02949,2461139.8086,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-02949 20260409.3086 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J303.5450+37.7260,2461139.8086,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J303.5450+37.7260 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J295.9948+34.0220,2461139.8086,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J295.9948+34.0220 20260409.3086 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2055647218487817856,2461139.8086,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 2055647218487817856 20260409.3086 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2055619932539580032,2461139.8086,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 2055619932539580032 20260409.3086 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2054969541357745664,2461139.8086,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 2054969541357745664 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2054977615899132672,2461139.8086,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 2054977615899132672 20260409.3086 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2055405459049131520,2461139.8086,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 2055405459049131520 20260409.3086 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0493 Cyg,2461139.8086,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0493 Cyg 20260409.3086 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J303.1657+33.0123,2461139.8086,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J303.1657+33.0123 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J302.9720+32.8011,2461139.8086,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J302.9720+32.8011 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0434 Cyg,2461139.8086,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0434 Cyg 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J303.5984+36.1625,2461139.8086,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J303.5984+36.1625 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2068623616040782080,2461139.8086,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 2068623616040782080 20260409.3086 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J286.2462+35.0295,2461139.8086,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J286.2462+35.0295 20260409.3086 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J301.0102+38.4252,2461139.8086,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J301.0102+38.4252 20260409.3086 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J303.1375+34.3897,2461139.8086,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J303.1375+34.3897 20260409.3086 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J294.6004+40.8860,2461139.8086,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J294.6004+40.8860 20260409.3086 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J303.3473+33.1992,2461139.8086,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J303.3473+33.1992 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J295.7289+37.7022,2461139.8086,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J295.7289+37.7022 20260409.3086 13.19CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2102441230756464128,2461139.8086,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 2102441230756464128 20260409.3086 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J200009.20+392506.2,2461139.8086,13.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J200009.20+392506.2 20260409.3086 13.27CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0984 Cyg,2461139.8086,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0984 Cyg 20260409.3086 13.19CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J289.7940+35.3062,2461139.8086,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J289.7940+35.3062 20260409.3086 13.46CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J201124.46+375424.0,2461139.8086,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J201124.46+375424.0 20260409.3086 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J200849.07+390431.4,2461139.8086,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J200849.07+390431.4 20260409.3086 13.66CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1361 Cyg,2461139.8086,13.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1361 Cyg 20260409.3086 13.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-05184,2461139.8086,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-05184 20260409.3086 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J192318.96+350146.9,2461139.8086,13.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J192318.96+350146.9 20260409.3086 13.23CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-04022,2461139.8086,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-04022 20260409.3086 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2034881841905310592,2461139.8086,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 2034881841905310592 20260409.3086 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J288.0498+37.3047,2461139.8086,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J288.0498+37.3047 20260409.3086 13.29CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-02504,2461139.8086,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-02504 20260409.3086 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-00839,2461139.8086,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-00839 20260409.3086 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J201124.13+381718.6,2461139.8086,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J201124.13+381718.6 20260409.3086 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-04278,2461139.8086,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-04278 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461139.8086,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260409.3086 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1274 Cyg,2461139.8086,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1274 Cyg 20260409.3086 11.64CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461139.8086,13.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260409.3086 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2055419550859618688,2461139.8086,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 2055419550859618688 20260409.3086 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-04294,2461139.8086,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-04294 20260409.3086 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-01181,2461139.8086,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-01181 20260409.3086 11.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J192500+3754.2,2461139.8086,13.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J192500+3754.2 20260409.3086 13.43CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J192505.02+330633.3,2461139.8086,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J192505.02+330633.3 20260409.3086 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J293.6843+34.2203,2461139.8086,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J293.6843+34.2203 20260409.3086 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J192944.15+331035.0,2461139.8086,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J192944.15+331035.0 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-01770,2461139.8086,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-01770 20260409.3086 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1278 Cyg,2461139.8086,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1278 Cyg 20260409.3086 12.71CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-04554,2461139.8086,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-04554 20260409.3086 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V2217 Cyg,2461139.8086,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V2217 Cyg 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Mis V1093,2461139.8086,13.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 V1093 20260409.3086 13.23CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-07104,2461139.8086,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-07104 20260409.3086 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1439 Cyg,2461139.8086,9.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1439 Cyg 20260409.3086 9.93CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J201211.26+392618.8,2461139.8086,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J201211.26+392618.8 20260409.3086 13.15CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-04161,2461139.8086,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-04161 20260409.3086 12.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J193106.76+330713.4,2461139.8086,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J193106.76+330713.4 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0431 Cyg,2461139.8086,9.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0431 Cyg 20260409.3086 9.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 8294401,2461139.8086,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 8294401 20260409.3086 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J195519+4132.2,2461139.8086,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J195519+4132.2 20260409.3086 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1152 Cyg,2461139.8086,10.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1152 Cyg 20260409.3086 10.12CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-07932,2461139.8086,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-07932 20260409.3086 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-03473,2461139.8086,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-03473 20260409.3086 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2073220609747137664,2461139.8086,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 2073220609747137664 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2098978559402980224,2461139.8086,12.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 2098978559402980224 20260409.3086 12.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-18487,2461139.8086,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-18487 20260409.3086 12.96CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-08104,2461139.8086,12.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-08104 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-02503,2461139.8086,13.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-02503 20260409.3086 13.27CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2014289+350632,2461139.8086,11.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J2014289+350632 20260409.3086 11.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-08314,2461139.8086,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-08314 20260409.3086 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J303.0933+37.3200,2461139.8086,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J303.0933+37.3200 20260409.3086 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 09.3086 2461139.8086 12.73 20:12:06.40 +35:03:11.6
72.71487 0.61361 galactic Cyg Second-epoch detections are separated by 1.0" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 2058850061475101696 | 20:12:06.40 +35:03:11.6 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 2058850061475101696,2461139.8086,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 2058850061475101696 20260409.3086 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-02764,2461139.8086,12.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-02764 20260409.3086 12.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1915507+363222,2461139.8086,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J1915507+363222 20260409.3086 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-00212,2461139.8086,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-00212 20260409.3086 11.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-05667,2461139.8086,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-05667 20260409.3086 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J195642.19+370028.3,2461139.8086,12.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J195642.19+370028.3 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J303.3146+35.7068,2461139.8086,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J303.3146+35.7068 20260409.3086 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J194146.27+330119.1,2461139.8086,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J194146.27+330119.1 20260409.3086 12.71CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0969 Cyg,2461139.8086,11.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0969 Cyg 20260409.3086 11.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J195021.54+333132.8,2461139.8086,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J195021.54+333132.8 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-03925,2461139.8086,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-03925 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J294.8102+33.7621,2461139.8086,13.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J294.8102+33.7621 20260409.3086 13.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ROTSE1 J193233.48+404510.7,2461139.8086,13.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ROTSE1 J193233.48+404510.7 20260409.3086 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2055651749653738112,2461139.8086,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 2055651749653738112 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J195009.53+364641.8,2461139.8086,12.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J195009.53+364641.8 20260409.3086 12.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
KS Cyg,2461139.8086,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
KS Cyg 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J194203.59+343231.3,2461139.8086,13.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J194203.59+343231.3 20260409.3086 13.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J291.1659+33.7093,2461139.8086,12.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J291.1659+33.7093 20260409.3086 12.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2059933213581055360,2461139.8086,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 2059933213581055360 20260409.3086 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J193702.50+340312.6,2461139.8086,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J193702.50+340312.6 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-13859,2461139.8086,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-13859 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J193446.47+351328.7,2461139.8086,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J193446.47+351328.7 20260409.3086 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J293.6479+33.6939,2461139.8086,12.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J293.6479+33.6939 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-03405,2461139.8086,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-03405 20260409.3086 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2007329+372146,2461139.8086,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J2007329+372146 20260409.3086 12.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0942 Cyg,2461139.8086,11.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0942 Cyg 20260409.3086 11.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-01728,2461139.8086,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-01728 20260409.3086 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J200537.07+345330.9,2461139.8086,11.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J200537.07+345330.9 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.8086,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.3086 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2047604428375772416,2461139.8086,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 2047604428375772416 20260409.3086 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-03157,2461139.8086,12.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-03157 20260409.3086 12.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0421 Cyg,2461139.8086,12.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0421 Cyg 20260409.3086 12.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-02579,2461139.8086,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-02579 20260409.3086 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J195823.17+353418.5,2461139.8086,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J195823.17+353418.5 20260409.3086 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-03379,2461139.8086,12.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-03379 20260409.3086 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-02674,2461139.8086,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-02674 20260409.3086 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-02926,2461139.8086,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-02926 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J286.5148+35.9381,2461139.8086,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J286.5148+35.9381 20260409.3086 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-00009,2461139.8086,10.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-00009 20260409.3086 10.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2059052062409040640,2461139.8086,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 2059052062409040640 20260409.3086 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J192906+3747.3,2461139.8086,11.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J192906+3747.3 20260409.3086 11.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 8453804,2461139.8086,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 8453804 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2055722535028275456,2461139.8086,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 2055722535028275456 20260409.3086 11.63CV 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J297.6409+34.5261,2461139.8086,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J297.6409+34.5261 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-00433,2461139.8086,10.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-00433 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-00742,2461139.8086,11.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-00742 20260409.3086 11.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461139.8086,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260409.3086 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1300 Cyg,2461139.8086,11.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1300 Cyg 20260409.3086 11.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-00485,2461139.8086,11.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-00485 20260409.3086 11.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-13263,2461139.8086,13.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-13263 20260409.3086 13.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J194208.21+332340.3,2461139.8086,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J194208.21+332340.3 20260409.3086 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-03469,2461139.8086,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-03469 20260409.3086 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
TSVSC1 TN-N030132122-59-67-2,2461139.8086,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
TSVSC1 TN-N030132122-59-67-2 20260409.3086 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSV 12302,2461139.8086,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 12302 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-02316,2461139.8086,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-02316 20260409.3086 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
2MASS J20081213+3536060,2461139.8086,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
2MASS J20081213+3536060 20260409.3086 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J201319.73+325725.1,2461139.8086,11.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J201319.73+325725.1 20260409.3086 11.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J191930.87+332738.3,2461139.8086,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J191930.87+332738.3 20260409.3086 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J195408+4040.8,2461139.8086,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J195408+4040.8 20260409.3086 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.6734+34.7630,2461139.8086,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J299.6734+34.7630 20260409.3086 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J193749.39+332322.0,2461139.8086,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J193749.39+332322.0 20260409.3086 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-03939,2461139.8086,12.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-03939 20260409.3086 12.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-06953,2461139.8086,12.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-06953 20260409.3086 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J201121.87+344559.1,2461139.8086,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J201121.87+344559.1 20260409.3086 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-03185,2461139.8086,12.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-03185 20260409.3086 12.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-07755,2461139.8086,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-07755 20260409.3086 13.21CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-02707,2461139.8086,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-02707 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSV 12209,2461139.8086,12.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 12209 20260409.3086 12.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J194741.77+343600.2,2461139.8086,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J194741.77+343600.2 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-10779,2461139.8086,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-10779 20260409.3086 13.09CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0740 Cyg,2461139.8086,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0740 Cyg 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GSC 02678-02168,2461139.8086,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GSC 02678-02168 20260409.3086 11.77CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1902401+353821,2461139.8086,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J1902401+353821 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J193756+4012.0,2461139.8086,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J193756+4012.0 20260409.3086 12.99CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
KIC 6148249,2461139.8086,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
KIC 6148249 20260409.3086 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-04094,2461139.8086,13.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-04094 20260409.3086 13.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J296.3209+39.5093,2461139.8086,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J296.3209+39.5093 20260409.3086 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2055745693500320640,2461139.8086,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 2055745693500320640 20260409.3086 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-02766,2461139.8086,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-02766 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-14951,2461139.8086,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-14951 20260409.3086 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J192710.39+331804.3,2461139.8086,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J192710.39+331804.3 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J295.6761+35.2785,2461139.8086,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J295.6761+35.2785 20260409.3086 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-00396,2461139.8086,10.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-00396 20260409.3086 10.63CV 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0433 Cyg,2461139.8086,12.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0433 Cyg 20260409.3086 12.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J194155.41+330420.3,2461139.8086,12.33,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J194155.41+330420.3 20260409.3086 12.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J192816.95+330112.4,2461139.8086,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J192816.95+330112.4 20260409.3086 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J194749.46+341443.4,2461139.8086,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J194749.46+341443.4 20260409.3086 11.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-03025,2461139.8086,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-03025 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0698 Cyg,2461139.8086,11.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0698 Cyg 20260409.3086 11.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J193151+4245.1,2461139.8086,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J193151+4245.1 20260409.3086 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2058727191070536960,2461139.8086,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 2058727191070536960 20260409.3086 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1934268+370049,2461139.8086,12.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J1934268+370049 20260409.3086 12.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0452 Cyg,2461139.8086,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0452 Cyg 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V2297 Cyg,2461139.8086,12.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V2297 Cyg 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1468 Cyg,2461139.8086,11.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1468 Cyg 20260409.3086 11.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J194835+4026.9,2461139.8086,11.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J194835+4026.9 20260409.3086 11.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2048971877229049088,2461139.8086,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 2048971877229049088 20260409.3086 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J195117.60+333039.8,2461139.8086,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J195117.60+333039.8 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2048084777506995072,2461139.8086,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 2048084777506995072 20260409.3086 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2060397177435097600,2461139.8086,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 2060397177435097600 20260409.3086 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-00673,2461139.8086,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-00673 20260409.3086 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J194516.50+330649.0,2461139.8086,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J194516.50+330649.0 20260409.3086 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.8086,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.3086 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-02089,2461139.8086,11.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-02089 20260409.3086 11.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J297.8330+37.3082,2461139.8086,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J297.8330+37.3082 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-01293,2461139.8086,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-01293 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 8266192,2461139.8086,12.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 8266192 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-06955,2461139.8086,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-06955 20260409.3086 12.99CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0375 Lyr,2461139.8086,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0375 Lyr 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J302.4415+38.4110,2461139.8086,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J302.4415+38.4110 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-02930,2461139.8086,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-02930 20260409.3086 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J295.1565+35.8344,2461139.8086,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J295.1565+35.8344 20260409.3086 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1294 Cyg,2461139.8086,11.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1294 Cyg 20260409.3086 11.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-07141,2461139.8086,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-07141 20260409.3086 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-06830,2461139.8086,13.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-06830 20260409.3086 13.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0893 Cyg,2461139.8086,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0893 Cyg 20260409.3086 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Mis V1100,2461139.8086,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 V1100 20260409.3086 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.8086,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.3086 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J302.5294+33.9273,2461139.8086,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J302.5294+33.9273 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1908094+354005,2461139.8086,12.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J1908094+354005 20260409.3086 12.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461139.8086,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260409.3086 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0497 Lyr,2461139.8086,12.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0497 Lyr 20260409.3086 12.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 8460806,2461139.8086,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 8460806 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-15265,2461139.8086,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-15265 20260409.3086 13.15CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2010347+332727,2461139.8086,11.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J2010347+332727 20260409.3086 11.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2034402076891269632,2461139.8086,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 2034402076891269632 20260409.3086 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
TSVSC1 TN-N030303021-4-67-2,2461139.8086,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
TSVSC1 TN-N030303021-4-67-2 20260409.3086 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
Mean magnitude and position on the discovery images:
2026 04 09.3086 2461139.8086 12.05 20:14:37.70 +35:26:28.2
73.32261 0.39855 galactic Cyg Second-epoch detections are separated by 0.9" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 2055888939242278656 | 20:14:37.91 +35:26:28.4 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=1.199+/-0.035 (M)
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 2055888939242278656,2461139.8086,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 2055888939242278656 20260409.3086 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-09945,2461139.8086,12.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-09945 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J200158.21+392119.2,2461139.8086,12.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J200158.21+392119.2 20260409.3086 12.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-01588,2461139.8086,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-01588 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-02019,2461139.8086,12.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-02019 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-00905,2461139.8086,11.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-00905 20260409.3086 11.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.8086,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-03156,2461139.8086,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-03156 20260409.3086 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J296.4740+35.5647,2461139.8086,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J296.4740+35.5647 20260409.3086 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1950076+332058,2461139.8086,10.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J1950076+332058 20260409.3086 10.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J201208.50+355613.5,2461139.8086,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J201208.50+355613.5 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 8436298,2461139.8086,11.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 8436298 20260409.3086 11.63CV 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1823 Cyg,2461139.8086,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1823 Cyg 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-09951,2461139.8086,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-09951 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-06637,2461139.8086,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-06637 20260409.3086 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-09171,2461139.8086,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-09171 20260409.3086 13.12CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
CzeV3036,2461139.8086,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CzeV3036 20260409.3086 11.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS 8446510,2461139.8086,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 8446510 20260409.3086 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-04708,2461139.8086,12.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-04708 20260409.3086 12.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J194420.49+395249.8,2461139.8086,12.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J194420.49+395249.8 20260409.3086 12.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1999 Cyg,2461139.8086,12.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1999 Cyg 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2055418863664791168,2461139.8086,11.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 2055418863664791168 20260409.3086 11.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-00422,2461139.8086,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-00422 20260409.3086 11.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2058939843505153152,2461139.8086,12.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 2058939843505153152 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-05094,2461139.8086,13.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-05094 20260409.3086 13.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-07892,2461139.8086,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-07892 20260409.3086 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-02876,2461139.8086,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-02876 20260409.3086 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J295.9777+40.1036,2461139.8086,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J295.9777+40.1036 20260409.3086 12.97CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-05061,2461139.8086,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-05061 20260409.3086 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-01072,2461139.8086,11.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-01072 20260409.3086 11.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-08612,2461139.8086,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-08612 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J301.5450+33.6051,2461139.8086,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J301.5450+33.6051 20260409.3086 12.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Mis V0123,2461139.8086,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 V0123 20260409.3086 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2073129178485689600,2461139.8086,12.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 2073129178485689600 20260409.3086 12.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-06583,2461139.8086,12.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-06583 20260409.3086 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-10793,2461139.8086,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-10793 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J285.4287+42.2939,2461139.8086,13.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J285.4287+42.2939 20260409.3086 13.34CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J200353.72+334654.5,2461139.8086,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J200353.72+334654.5 20260409.3086 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2011083+390656,2461139.8086,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J2011083+390656 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J201552.08+385113.1,2461139.8086,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J201552.08+385113.1 20260409.3086 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2060490257969733504,2461139.8086,11.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 2060490257969733504 20260409.3086 11.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J200915.95+370147.2,2461139.8086,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J200915.95+370147.2 20260409.3086 12.99CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J192731+3934.0,2461139.8086,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J192731+3934.0 20260409.3086 13.21CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J292.7025+38.9564,2461139.8086,11.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J292.7025+38.9564 20260409.3086 11.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V2295 Cyg,2461139.8086,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V2295 Cyg 20260409.3086 12.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J300.8678+40.5666,2461139.8086,12.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J300.8678+40.5666 20260409.3086 12.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-02059,2461139.8086,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-02059 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J201405.09+401245.8,2461139.8086,12.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J201405.09+401245.8 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J190548.00+333629.6,2461139.8086,11.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J190548.00+333629.6 20260409.3086 11.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J296.1172+34.3281,2461139.8086,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J296.1172+34.3281 20260409.3086 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1946187+350348,2461139.8086,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J1946187+350348 20260409.3086 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2074082897435772672,2461139.8086,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 2074082897435772672 20260409.3086 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
KIC 7050754,2461139.8086,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
KIC 7050754 20260409.3086 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1511 Cyg,2461139.8086,11.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1511 Cyg 20260409.3086 11.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-08101,2461139.8086,13.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-08101 20260409.3086 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J299.4192+36.0191,2461139.8086,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J299.4192+36.0191 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-03636,2461139.8086,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-03636 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HAT 199-03000,2461139.8086,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 199-03000 20260409.3086 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J201300.03+332639.7,2461139.8086,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J201300.03+332639.7 20260409.3086 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
2MASS J20100064+3651114,2461139.8086,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
2MASS J20100064+3651114 20260409.3086 12.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461098.98950343 27.02.2026 11:44:43.096 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
First image: 2461098.98950343 27.02.2026 11:44:43.096 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
Last image: 2461139.80896990 09.04.2026 07:24:44.999 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 89
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.88
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 10 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): 35696
Objects passed selection criteria: 35636
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 31245
Average stars matched: 30102 (96.3418 %)
Memory usage VmPeak: 136780 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 9 02:26:55 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: 2461098.98950343 27.02.2026 11:44:43.096 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
First image: 2461098.98950343 27.02.2026 11:44:43.096 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
Last image: 2461139.80896990 09.04.2026 07:24:44.999 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 797
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.55
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: 107 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): 270195
Objects passed selection criteria: 269458
Measurements per detected object (mean, median, min, max): 2.9 3.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 3.0 2 4
Average stars detected per image: 212568
Average stars matched: 203449 (95.7097 %)
Memory usage VmPeak: 2079940 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 9 02:33:58 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/TTUQ1b1x1/TTUQ1_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 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits
SExtractor catalog cache: saved Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat to cache
SExtractor catalog cache: saved Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.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-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461139.80823208
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-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits exists and is non-empty
Saving wcs_Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits to local_wcs_cache/
'wcs_Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits' -> 'local_wcs_cache/wcs_Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits'
wcs_Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits exists and is non-empty
Saving wcs_Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits to local_wcs_cache/
'wcs_Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits' -> 'local_wcs_cache/wcs_Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits'
wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits exists and is non-empty
Saving wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits to local_wcs_cache/
'wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits' -> 'local_wcs_cache/wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits'
wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits exists and is non-empty
Saving wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits to local_wcs_cache/
'wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits' -> 'local_wcs_cache/wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits'
The image scale is 5.92"/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 19:38:24.380 +37:59:43.16
Second-epoch image center 19:38:11.248 +38:00:02.37
Angular distance between the image centers 0.0434 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 19:38:24.380 +37:59:43.16
Second-epoch image center 19:38:09.164 +38:00:31.09
Angular distance between the image centers 0.0517 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 19:38:11.248 +38:00:02.37
Second-epoch second image center 19:38:09.164 +38:00:31.09
Angular distance between the image centers 0.01051 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-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits &> /tmp/tmp.UfQyZU6Jor
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits &> /tmp/tmp.Uqvg58xhUC
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits &> /tmp/tmp.OSor9EFpIx
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits &> /tmp/tmp.ZAcM0Yb49L
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.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-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits and wcs_Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.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-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits and wcs_Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat
Found non-empty wcs_Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits and wcs_Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat
The reference image (wcs_Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits) and catalog (wcs_Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat) found
'wcs_Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat' -> 'wcsmag.cat'
Read 36462 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 283.6157 to 305.0045 deg, Dec +32.0124 to +43.3705 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 283.6157 to 305.0045 deg, Dec 32.0124 to 43.3705 deg
Loaded 31163 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): 1986 out of 2233 total matches.
Matched with Tycho-2 2233 out of 36462 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.869053
a=0.000000 b=1.000000 c=22.869053
From vast_summary.log: estimated ref. image limiting mag.: -7.88
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.99
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.99
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 79 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
2.2 pix Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
4.4 pix fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits
4.4 pix fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits
Limiting magnitude estimates:
15.0 mag. Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
15.0 mag. Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
14.2 mag. fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits
14.2 mag. fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits
All-image limiting magnitude estimate: 14.2 (SNR ) 11.7 (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.UfQyZU6Jor (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.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-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits' -> 'wcs_Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
WCS_IMAGE_NAME=wcs_Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
WCS-calibrated image found: wcs_Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
Checking if the catalog wcs_Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat corresponding to the image wcs_Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits alredy exist and is non-empty...
Catalog wcs_Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat corresponding to the image wcs_Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
WCS catalog name: wcs_Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=4454, passed=36462
Got 36462 stars (including 31968 good ones) from the SExtractor catalog wcs_Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat
util/solve_plate_with_UCAC5 got 36462 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.5'
Seting catalog search parameters based on the expected field of view 944.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013118 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010494 (37.8 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 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 851 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 826 matched stars entering correct_measured_positions(), 776 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.11"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 825 matched stars entering correct_measured_positions(), 29935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.35"
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 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 920 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 898 matched stars entering correct_measured_positions(), 29961 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.32"
Accuracy estimation diagnostic: 896 matched stars entering correct_measured_positions(), 31122 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.30"
Excluding outliers - 896 stars left (next iteration limit 907)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits -region wcs_Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.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.Uqvg58xhUC (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.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-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits' -> 'wcs_Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
WCS_IMAGE_NAME=wcs_Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
WCS-calibrated image found: wcs_Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
Checking if the catalog wcs_Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits.cat corresponding to the image wcs_Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits alredy exist and is non-empty...
Catalog wcs_Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits.cat corresponding to the image wcs_Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
WCS catalog name: wcs_Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=4450, passed=36391
Got 36391 stars (including 31905 good ones) from the SExtractor catalog wcs_Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits.cat
util/solve_plate_with_UCAC5 got 36391 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.8'
Seting catalog search parameters based on the expected field of view 944.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013122 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010498 (37.8 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 32.0 to 43.4)
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...
Accuracy estimation diagnostic: 902 matched stars entering correct_measured_positions(), 879 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.15"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 901 matched stars entering correct_measured_positions(), 30485 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.19"
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 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 924 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 913 matched stars entering correct_measured_positions(), 30490 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.17"
Accuracy estimation diagnostic: 912 matched stars entering correct_measured_positions(), 30730 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.12"
Excluding outliers - 912 stars left (next iteration limit 991)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits -region wcs_Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.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.OSor9EFpIx (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits
WCS-calibrated image found: wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits
Checking if the catalog wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits.cat corresponding to the image wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits.cat corresponding to the image wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits
WCS catalog name: wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1858, passed=26337
Got 26337 stars (including 24473 good ones) from the SExtractor catalog wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits.cat
util/solve_plate_with_UCAC5 got 26337 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.5'
Seting catalog search parameters based on the expected field of view 942.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013090 (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 0.010472 (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 609 to 669 (Dec 31.9 to 43.4)
Done reading UCAC5 zone files...
Matched 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 913 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 25630 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
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 609 to 669 (Dec 31.9 to 43.4)
Done reading UCAC5 zone files...
Matched 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 25630 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 25630 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Excluding outliers - 930 stars left (next iteration limit 1023)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits -region wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.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.ZAcM0Yb49L (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits
WCS-calibrated image found: wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits
Checking if the catalog wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits.cat corresponding to the image wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits.cat corresponding to the image wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits
WCS catalog name: wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1885, passed=26529
Got 26529 stars (including 24639 good ones) from the SExtractor catalog wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits.cat
util/solve_plate_with_UCAC5 got 26529 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.5'
Seting catalog search parameters based on the expected field of view 942.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013090 (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 0.010472 (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 609 to 669 (Dec 31.9 to 43.4)
Done reading UCAC5 zone files...
Matched 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 911 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 25816 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 609 to 669 (Dec 31.9 to 43.4)
Done reading UCAC5 zone files...
Matched 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 25816 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Accuracy estimation diagnostic: 930 matched stars entering correct_measured_positions(), 25816 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Excluding outliers - 930 stars left (next iteration limit 1023)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits -region wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.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-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/wcs_Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits'
Saving fully-calibrated image wcs_Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/wcs_Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits'
Saving fully-calibrated image wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits'
Saving fully-calibrated image wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits'
Preparing the HTML report for the field Cyg-05-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out08104.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out12085.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out51422.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53263.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53360.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53574.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53696.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53731.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53751.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53763.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53769.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53845.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53852.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53856.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53866.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53878.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53920.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53954.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53961.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53969.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53978.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53991.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53993.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53995.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53997.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54010.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54015.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54029.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54034.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54038.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54051.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54061.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54072.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54075.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54106.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54113.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54118.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54120.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54128.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54129.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54131.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54139.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54140.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54142.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54152.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out54155.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out07389.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12113.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out13120.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14113.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16918.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19089.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19412.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24834.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28299.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36087.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53303.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53888.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54076.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 19s
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: 6s
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Considering the candidate 52789_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 52789_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:19:20.78 +41:23:30.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 52922_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 52922_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:12:11.97 +33:03:34.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52935_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 52935_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:41.21 +33:18:46.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52947_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 52947_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:20:08.76 +41:40:57.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53085_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 53085_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:19.82 +33:00:35.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53112_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 53112_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:44:09.62 +39:47:22.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53127_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 53127_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:12:44.57 +33:03:00.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53263_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 53263_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:17:25.86 +42:48:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.08, MAG_FAINT_SEARCH_LIMIT=12.06)GAIADR2_OUTPUT=# 2.981 2102732429540468736 289.35746942716 +42.81391305759 10.7642 9.6039 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.981#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53282_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 53282_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:17.54 +33:06:24.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53303_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 53303_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 53360_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 53360_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:45:25.75 +40:15:38.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.13, MAG_FAINT_SEARCH_LIMIT=12.11)GAIADR2_OUTPUT=# 2.525 2076361811386328832 296.35735135977 +40.26125537659 10.1950 8.6733 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.525#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53432_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 53432_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:12:53.56 +32:56:11.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53475_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 53475_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:14:07.30 +33:48:58.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53574_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 53574_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:40:59.00 +36:43:29.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.43, MAG_FAINT_SEARCH_LIMIT=12.41)GAIADR2_OUTPUT=# 3.466 2048700263499926144 295.24598296508 +36.72576086714 10.1762 8.4075 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.466#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53696_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 53696_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:59:53.46 +36:16:36.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.49, MAG_FAINT_SEARCH_LIMIT=12.47)GAIADR2_OUTPUT=# 3.516 2059732282164923392 299.97227277360 +36.27775881520 11.3978 10.7712 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.516#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53731_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 53731_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:03:18.46 +35:07:55.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.50, MAG_FAINT_SEARCH_LIMIT=12.48)GAIADR2_OUTPUT=# 2.014 2058678434605772288 300.82759885566 +35.13198516519 10.6415 9.4037 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.014#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53751_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 53751_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:30:36.75 +39:45:45.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.71, MAG_FAINT_SEARCH_LIMIT=12.69)GAIADR2_OUTPUT=# 1.313 2053194173673227776 292.65321908187 +39.76299634015 11.2897 10.3213 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.313#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53755_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 53755_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:33:41.94 +38:47:20.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 53763_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 53763_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:12.38 +32:50:40.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.43, MAG_FAINT_SEARCH_LIMIT=12.41)
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Considering the candidate 53769_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 53769_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:26:02.17 +35:03:06.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.67, MAG_FAINT_SEARCH_LIMIT=12.65)GAIADR2_OUTPUT=# 3.454 2049763143333038592 291.50801364461 +35.05223880695 12.2317 10.3946 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.454#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53845_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 53845_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:15:50.47 +36:32:21.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.80, MAG_FAINT_SEARCH_LIMIT=12.78)GAIADR2_OUTPUT=# 2.038 2051109705780203264 288.95988070950 +36.53965419361 10.9384 9.6484 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.038#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53852_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 53852_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:42:28.35 +37:40:12.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.74, MAG_FAINT_SEARCH_LIMIT=12.72)GAIADR2_OUTPUT=# 3.544 2049033896558204416 295.61691139907 +37.67038215156 11.7229 11.2143 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.544#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53856_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 53856_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:02:58.48 +41:05:06.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.74, MAG_FAINT_SEARCH_LIMIT=12.72)GAIADR2_OUTPUT=# 3.827 2074416088131126912 300.74380540181 +41.08619687403 10.3999 8.8872 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.827#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53866_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 53866_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:15:45.53 +37:20:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.80, MAG_FAINT_SEARCH_LIMIT=12.78)GAIADR2_OUTPUT=# 2.238 2051218759290512896 288.93939242529 +37.34701307609 10.9605 9.6871 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.238#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53878_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 53878_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:07:19.39 +42:16:36.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.76, MAG_FAINT_SEARCH_LIMIT=12.74)GAIADR2_OUTPUT=# 3.122 2074964263390345088 301.83127840053 +42.27748334364 11.0215 9.6410 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.122#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53888_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 53888_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 53920_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 53920_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:41:39.66 +37:07:56.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.73, MAG_FAINT_SEARCH_LIMIT=12.71)GAIADR2_OUTPUT=# 2.234 2048808221799389824 295.41509456457 +37.13283030213 11.1108 9.9694 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.234#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53954_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 53954_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:19.44 +32:57:25.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.62, MAG_FAINT_SEARCH_LIMIT=12.60)GAIADR2_OUTPUT=# 3.646 2054974867117112448 303.33219448225 +32.95696505280 11.0265 9.7144 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.646#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53961_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 53961_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:12:26.62 +35:48:53.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.84, MAG_FAINT_SEARCH_LIMIT=12.82)GAIADR2_OUTPUT=# 3.442 2050597539522761600 288.11138654429 +35.81559898689 11.9465 11.2384 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.442#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53969_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 53969_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:28:59.12 +37:46:26.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.85, MAG_FAINT_SEARCH_LIMIT=12.83)GAIADR2_OUTPUT=# 2.420 2051886265926288512 292.24609414141 +37.77475612048 11.5535 10.7219 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.420#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53978_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 53978_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:32:08.17 +37:48:54.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 2.931 2051856342898037888 293.03385029238 +37.81585554590 11.7289 11.3707 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.931#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53991_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 53991_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:13:57.56 +41:44:44.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 2.437 2102284859587534720 288.48978315682 +41.74625921259 12.1072 11.6723 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.437#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53993_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 53993_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:02:56.34 +39:46:44.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 1.907 2100342194338866304 285.73465962728 +39.77944182326 11.8040 10.8294 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.907#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53995_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 53995_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:18:55.99 +38:42:54.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 1.955 2052890983337277056 289.73322971965 +38.71573544514 11.8156 11.3891 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.955#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53997_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 53997_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:23:22.39 +38:11:10.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 2.749 2052616582169356160 290.84348407798 +38.18705410334 11.9846 11.5534 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.749#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54010_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 54010_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:06:14.75 +34:16:37.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.97, MAG_FAINT_SEARCH_LIMIT=12.95)GAIADR2_OUTPUT=# 5.186 2044414504603542528 286.56113122145 +34.27575174699 12.0446 11.3415 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.186#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54015_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 54015_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:05:13.18 +35:13:04.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.99, MAG_FAINT_SEARCH_LIMIT=12.97)GAIADR2_OUTPUT=# 1.811 2092635713041282560 286.30470980175 +35.21841816742 11.9135 11.3862 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.811#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54029_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 54029_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:11:08.33 +40:46:02.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.08, MAG_FAINT_SEARCH_LIMIT=13.06)GAIADR2_OUTPUT=# 0.329 2100629785350150272 287.78458946619 +40.76728988614 12.0939 11.3816 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.329#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54034_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 54034_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:08:38.18 +38:09:34.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 2.028 2099167469244796544 287.15869016041 +38.15991543111 10.8224 9.4424 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.028#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54038_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 54038_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:14:22.89 +34:00:34.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.99, MAG_FAINT_SEARCH_LIMIT=12.97)GAIADR2_OUTPUT=# 2.771 2049491667040586496 288.59596358693 +34.00896020419 11.8339 10.7963 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.771#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54051_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 54051_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:10:32.45 +35:27:00.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 1.619 2050574140540348416 287.63499779529 +35.45058229693 11.5333 10.3992 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.619#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54061_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 54061_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:21:49.84 +42:32:50.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 2.484 2101998226348450560 290.45751034370 +42.54812479647 11.8264 10.9650 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.484#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54072_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 54072_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:02:58.41 +39:58:53.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 2.541 2100722724141169280 285.74292828379 +39.98203393756 11.9697 11.1173 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.541#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54075_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 54075_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:31:47.52 +42:07:23.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)
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Considering the candidate 54076_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 54076_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 54106_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 54106_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:04:34.53 +35:25:10.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 2.241 2092653442666272256 286.14373808386 +35.42030686427 12.0586 11.6985 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.241#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54113_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 54113_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:02:11.78 +34:54:01.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 2.140 2092542460713080960 285.54881900244 +34.90099799598 12.0073 11.3393 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.140#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54118_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 54118_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:26:33.53 +41:56:32.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 1.549 2101742933492427904 291.63952337445 +41.94287995655 12.0077 11.6344 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.549#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54120_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 54120_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:19:32.54 +39:20:05.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 2.272 2100982831662296832 289.88545774162 +39.33540125344 11.5839 10.5462 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.272#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54128_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 54128_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:10:44.72 +36:58:08.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 0.172 2098847580081040768 287.68628622488 +36.96911295510 12.1801 11.6596 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.172#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54129_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 54129_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:34:49.71 +40:10:02.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 1.813 2053265122229971328 293.70691633808 +40.16769980591 11.7738 11.0038 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.813#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54131_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 54131_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:14:55.03 +35:37:07.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 1.669 2050488069397541632 288.72914002224 +35.61928019297 11.8911 11.1781 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.669#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54139_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 54139_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:04:47.34 +34:46:33.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 3.216 2044488309322119808 286.19821170144 +34.77547147875 12.2899 11.5803 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.216#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54140_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 54140_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:03:41.75 +34:15:42.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.08, MAG_FAINT_SEARCH_LIMIT=13.06)GAIADR2_OUTPUT=# 1.954 2044438109744068096 285.92365486379 +34.26237016620 11.9278 11.2100 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.954#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54142_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 54142_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:07:44.24 +35:15:45.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 1.193 2044612519775777408 286.93440037939 +35.26285460013 11.9739 11.2636 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.193#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54152_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 54152_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:06:06.78 +33:50:56.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 2.120 2044176730912597376 286.52831306964 +33.84972536975 12.1137 11.7567 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.120#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 54155_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 54155_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:10:15.89 +33:39:40.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.08, MAG_FAINT_SEARCH_LIMIT=13.06)GAIADR2_OUTPUT=# 1.390 2044214148667660928 287.56592606715 +33.66155636303 11.9505 11.1528 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.390#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 51422_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 51422_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:05:48.30 +33:36:30.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.34, MAG_FAINT_SEARCH_LIMIT=12.32)GAIADR2_OUTPUT=# 3.974 2044169515367534848 286.45000397207 +33.60817940523 10.4468 9.0125 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.974#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 16918_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 16918_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 13120_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 13120_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 12113_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 12113_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 15882_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 15882_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:32:55.90 +36:50:27.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 28299_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 28299_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 12085_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 12085_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:54:49.48 +35:55:52.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.52, MAG_FAINT_SEARCH_LIMIT=12.50)GAIADR2_OUTPUT=# 1.476 2059676134011030528 298.70641791027 +35.93152258582 10.5267 9.1234 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.476#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 12886_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 12886_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:00:13.32 +36:08:44.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 14113_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 14113_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 36087_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 36087_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 08104_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 08104_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:05:36.95 +34:53:30.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.35, MAG_FAINT_SEARCH_LIMIT=12.33)GAIADR2_OUTPUT=# 1.548 2058615762440603648 301.40447330618 +34.89191320304 10.6207 9.2681 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.548#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 07389_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 07389_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 04470_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 04470_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:13:01.42 +33:24:49.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 19412_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 19412_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 24834_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 24834_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28134_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 28134_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:19:53.68 +40:15:21.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 08914_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 08914_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:07:56.67 +34:29:11.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23089_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 23089_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:51:48.93 +39:00:35.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 19089_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 19089_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08074_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 08074_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:31:31.37 +34:42:16.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 03490_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 03490_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:46:25.62 +33:43:32.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 08308_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 08308_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:56:17.95 +35:05:03.1 in the exclusion list exclusion_list_bbsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 26s
Prepared the HTML report for the field Cyg-05-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
19:47:46.36 +34:42:07.2
20:03:33.00 +35:56:57.7
19:35:21.60 +36:04:03.3
19:24:57.98 +36:12:55.7
20:06:01.25 +37:14:30.0
19:53:32.84 +37:51:45.6
19:47:05.35 +37:55:42.3
19:55:13.31 +39:33:00.9
19:51:33.52 +40:39:37.4
19:48:26.68 +42:47:33.0
20:08:49.80 +35:30:51.7
19:29:08.06 +40:44:41.8
19:05:45.47 +37:04:10.9
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 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits
SExtractor catalog cache: saved Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat to cache
SExtractor catalog cache: saved Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.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-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
Creating symlink local_wcs_cache/wcs_Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits
Creating symlink local_wcs_cache/wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.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-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits exists and is non-empty
wcs_Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits exists and is non-empty
wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits exists and is non-empty
wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits exists and is non-empty
The image scale is 5.92"/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 19:38:24.380 +37:59:43.16
Second-epoch image center 19:38:11.248 +38:00:02.37
Angular distance between the image centers 0.0434 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 19:38:24.380 +37:59:43.16
Second-epoch image center 19:38:09.164 +38:00:31.09
Angular distance between the image centers 0.0517 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 19:38:11.248 +38:00:02.37
Second-epoch second image center 19:38:09.164 +38:00:31.09
Angular distance between the image centers 0.01051 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-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits &> /tmp/tmp.ehA4Joban0
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits &> /tmp/tmp.4zLcj7mMOI
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits &> /tmp/tmp.gfF8THl5iU
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits &> /tmp/tmp.GArZEQ4Ff8
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits
Calibrating the magnitude scale
Found non-empty wcs_Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.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-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits and wcs_Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.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-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits and wcs_Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat
Found non-empty wcs_Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits and wcs_Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat
The reference image (wcs_Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits) and catalog (wcs_Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat) found
'wcs_Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat' -> 'wcsmag.cat'
Read 289933 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 283.5863 to 305.0299 deg, Dec +31.9919 to +43.3713 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 283.5863 to 305.0299 deg, Dec 31.9919 to 43.3713 deg
Loaded 31292 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): 1391 out of 2470 total matches.
Matched with Tycho-2 2470 out of 289933 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.672267
a=0.000000 b=1.000000 c=22.672267
From vast_summary.log: estimated ref. image limiting mag.: -7.55
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.12
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.12
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 671 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
1.9 pix Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
3.9 pix fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits
3.9 pix fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits
Limiting magnitude estimates:
15.1 mag. Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
15.1 mag. Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
14.3 mag. fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits
14.3 mag. fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 13.5 (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.ehA4Joban0 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.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-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits' -> 'wcs_Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
WCS_IMAGE_NAME=wcs_Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
WCS-calibrated image found: wcs_Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
Checking if the catalog wcs_Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat corresponding to the image wcs_Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits alredy exist and is non-empty...
Catalog wcs_Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat corresponding to the image wcs_Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
WCS catalog name: wcs_Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat
SExtractor catalog parsing summary: zero_flux=2, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=64, blended=54567, passed=289867
Got 289867 stars (including 234945 good ones) from the SExtractor catalog wcs_Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat
util/solve_plate_with_UCAC5 got 289867 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.5'
Seting catalog search parameters based on the expected field of view 944.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013118 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010494 (37.8 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 609 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 836 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 811 matched stars entering correct_measured_positions(), 786 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.13"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 810 matched stars entering correct_measured_positions(), 259178 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.33"
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 609 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 909 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 887 matched stars entering correct_measured_positions(), 259200 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.33"
Accuracy estimation diagnostic: 887 matched stars entering correct_measured_positions(), 266743 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.35"
Excluding outliers - 887 stars left (next iteration limit 891)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits -region wcs_Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.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.4zLcj7mMOI (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.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-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits' -> 'wcs_Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
WCS_IMAGE_NAME=wcs_Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
WCS-calibrated image found: wcs_Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
Checking if the catalog wcs_Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits.cat corresponding to the image wcs_Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits alredy exist and is non-empty...
Catalog wcs_Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits.cat corresponding to the image wcs_Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
WCS catalog name: wcs_Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=90, blended=55059, passed=293463
Got 293463 stars (including 238031 good ones) from the SExtractor catalog wcs_Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits.cat
util/solve_plate_with_UCAC5 got 293463 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.8'
Seting catalog search parameters based on the expected field of view 944.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013122 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010498 (37.8 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 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 890 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 874 matched stars entering correct_measured_positions(), 854 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.07"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 872 matched stars entering correct_measured_positions(), 254104 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.15"
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 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 909 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 898 matched stars entering correct_measured_positions(), 254122 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 2.15"
Accuracy estimation diagnostic: 898 matched stars entering correct_measured_positions(), 260646 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.21"
Excluding outliers - 898 stars left (next iteration limit 959)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits -region wcs_Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.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.gfF8THl5iU (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits
WCS-calibrated image found: wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits
Checking if the catalog wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits.cat corresponding to the image wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits.cat corresponding to the image wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits
WCS catalog name: wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=26, blended=21902, passed=136046
Got 136046 stars (including 114064 good ones) from the SExtractor catalog wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits.cat
util/solve_plate_with_UCAC5 got 136046 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.5'
Seting catalog search parameters based on the expected field of view 942.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013090 (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 0.010472 (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 609 to 669 (Dec 31.9 to 43.4)
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 917 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 133388 with non-zero local correction accuracy
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 609 to 669 (Dec 31.9 to 43.4)
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 133391 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 133386 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Excluding outliers - 934 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits -region wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.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.GArZEQ4Ff8 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits
WCS_IMAGE_NAME=wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits
WCS-calibrated image found: wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits
Checking if the catalog wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits.cat corresponding to the image wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits alredy exist and is non-empty...
Catalog wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits.cat corresponding to the image wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits
WCS catalog name: wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=22161, passed=137056
Got 137056 stars (including 114806 good ones) from the SExtractor catalog wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits.cat
util/solve_plate_with_UCAC5 got 137056 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.5'
Seting catalog search parameters based on the expected field of view 942.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013090 (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 0.010472 (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 609 to 669 (Dec 31.9 to 43.5)
Done reading UCAC5 zone files...
Matched 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 916 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 133976 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
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 609 to 669 (Dec 31.9 to 43.5)
Done reading UCAC5 zone files...
Matched 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 133975 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 133973 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
Excluding outliers - 932 stars left (next iteration limit 1025)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits -region wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.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-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/wcs_Cyg-05-Q1b1x1_2026-02-27_05-44-43_20.00sec_-15.00C_LIGHT_0035.fits
Saving fully-calibrated image wcs_Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/wcs_Cyg-05-Q1b1x1_2026-02-27_05-45-35_20.00sec_-15.00C_LIGHT_0036.fits
Saving fully-calibrated image wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-23-41_20.00sec_-4.90C_LIGHTs_0186.fits
Saving fully-calibrated image wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Cyg-05-Q1b1x1_022542_TTUQ1b1x1_852_QoCKOkhX/wcs_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187.fits
Preparing the HTML report for the field Cyg-05-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out109436.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out111548.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out114081.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116539.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out131382.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out18022.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out182265.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out185106.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out194813.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20789.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out232967.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out300916.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out301091.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out301179.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out301347.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out301595.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out301619.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out301653.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out302138.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out302162.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out302384.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out302732.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out302754.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out304201.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out305022.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out305949.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out306145.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out306740.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out307609.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out308457.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out311071.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31271.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out327062.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328790.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328791.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328794.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328803.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328812.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328815.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328825.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328827.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328832.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328839.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328844.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328854.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328857.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328858.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328869.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328870.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328871.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328877.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328879.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328883.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328890.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328891.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328896.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328898.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328908.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328911.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328912.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328919.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328923.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328927.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328946.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328947.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328955.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328958.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328960.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328970.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328972.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328974.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328980.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328981.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328983.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328985.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328987.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328992.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328996.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out328997.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out329000.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out329004.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out329007.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out329011.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out329012.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out329022.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out329024.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out329026.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out329038.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out329039.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out329041.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out329043.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out329048.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out329052.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out329053.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out329058.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out329059.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out329063.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out329067.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out329068.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out329076.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out329077.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out329080.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out329081.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out329082.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out329083.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out329085.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out330140.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out330143.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out330195.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out330259.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out330287.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out330288.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out330345.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out330351.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out330405.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out330410.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out330472.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out330501.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out330605.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out330626.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out330679.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out330713.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out330741.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out330749.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out330785.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out330822.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out330860.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out330869.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out330882.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out330974.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out330989.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out330998.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out331018.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out331053.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out331106.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out331108.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out331121.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out331231.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out331232.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out331234.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out331252.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out331398.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out331442.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out331549.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out331621.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out331642.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out331821.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out331830.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out331842.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out331860.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out331871.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out331886.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out331887.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out331893.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out331903.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out331930.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out331935.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out331958.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out331981.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out332099.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out332165.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out332230.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out332239.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out332266.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out332299.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out332304.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out332311.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out332334.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out332350.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out332459.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out332461.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out332507.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out332518.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out332556.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out332576.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out332583.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out332587.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out332616.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out332628.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out332638.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out332688.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out332727.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out332761.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out332767.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out332784.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out332894.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out332917.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out332945.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out332955.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out332966.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out332974.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out333014.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out333039.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out333052.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out333073.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out333176.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out333199.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out333238.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out333242.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out333283.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out333288.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out333455.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out333473.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out333511.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out333538.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out333556.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out333569.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out333615.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out333774.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out333812.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out333912.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out333947.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out333981.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out334015.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out334030.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out334032.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out334036.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out334071.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out334105.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out334185.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out334200.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out334221.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out334249.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out334330.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out334352.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out334462.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out334566.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out334591.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out334605.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out334610.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out334743.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out334820.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out334917.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out334995.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out334998.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out335063.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out335159.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out335175.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out335186.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out335256.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out45702.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out46722.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out48990.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out60982.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out61872.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out62681.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out65878.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out71166.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out73270.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out04763.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out04799.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out07635.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09355.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out09994.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out100017.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out101309.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out102690.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103529.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103957.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out104664.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out107705.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out109021.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out110023.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out110172.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out111752.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out112623.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out113678.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out114759.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115059.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out115989.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118307.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118674.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118843.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out119025.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out119295.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out119998.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out120170.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out120333.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out120666.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out121038.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out121652.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12222.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out122243.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out125061.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out125538.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out126056.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out126280.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out126758.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out126901.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out12707.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out127418.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out127582.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out127787.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out128935.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out129076.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131470.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132952.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133806.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135087.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135872.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135937.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138528.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out138696.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out140668.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out142657.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out142778.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14305.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out143342.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out143467.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out148202.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out152505.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out153320.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15342.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15426.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15833.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15841.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out158551.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out158870.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out160836.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161477.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out161533.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out162928.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16389.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16491.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out16502.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out165109.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out165990.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out166578.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167637.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167956.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169010.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out170301.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out171075.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17213.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out172699.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173362.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out175381.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out179142.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out182293.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18255.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18399.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out185903.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out187029.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19013.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19017.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19198.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out192393.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19288.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out193423.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19533.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195579.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out197724.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out199627.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out19964.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out201305.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out202376.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out204948.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20497.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out207333.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out208211.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out209353.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21215.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out212675.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21315.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out216463.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out218572.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out219427.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out222033.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out222507.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out222848.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22446.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out226819.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22707.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out227622.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out229624.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out230836.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out231829.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234153.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out237125.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out24649.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out246854.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out248978.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out255055.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out260449.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27414.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out274160.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27474.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27959.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out286316.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288432.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out288606.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out289188.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29364.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29483.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29558.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out301615.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30235.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out302579.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out302939.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out303188.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out304603.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31823.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32043.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out328829.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out328843.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out328862.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out328873.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out328892.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out328894.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out328895.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out328897.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out328900.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out328906.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out328916.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out328935.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out328944.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out328948.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out328953.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out328954.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out328963.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out328964.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out328965.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out328973.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out328975.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out328977.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out328990.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out328994.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out329001.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out329006.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out329014.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out329021.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out329029.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out329034.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out329054.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out329056.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out329061.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out329062.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out329074.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out329084.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out330314.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out330847.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out330909.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out330949.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out331029.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out331465.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out331511.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out331590.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out331818.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out332197.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out332411.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out332485.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out332694.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out332916.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out332936.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out332950.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out333299.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out333488.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out333617.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out333675.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out333832.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out334089.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out334624.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out334881.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out33745.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34341.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34419.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34540.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35666.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36150.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36500.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38391.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38894.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39037.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39079.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39727.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41459.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out42197.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44167.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44412.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44553.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44867.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out44970.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45122.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46295.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46877.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out49728.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out49821.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out50541.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51578.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out51759.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52336.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52707.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53521.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54865.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55255.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55516.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55729.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55879.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56758.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56963.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57394.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out59158.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out60287.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out60354.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out60677.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65325.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65442.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65542.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66131.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67200.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68151.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68574.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out73311.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out73318.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out73680.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out73977.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out76628.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77385.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77969.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79539.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79858.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out81005.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out81331.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out81833.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out85005.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out86038.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out87178.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out87654.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out87981.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out89143.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out91449.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out92047.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out92326.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out92989.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out94725.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95139.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95549.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out95909.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out97337.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 185s
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: 145s
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Considering the candidate 328790_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 328790_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:04:21.45 +42:14:20.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)GAIADR2_OUTPUT=# 4.817 2104005732723435008 286.08946520171 +42.24036418923 13.9880 13.5437 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.817#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 328791_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 328791_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:06:55.85 +34:12:33.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.00, MAG_FAINT_SEARCH_LIMIT=14.98)GAIADR2_OUTPUT=# 2.001 2044400103573559168 286.73328486993 +34.20948011894 13.6502 13.2753 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.001#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 328794_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 328794_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:28:59.70 +41:05:36.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)
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Considering the candidate 328803_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 328803_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:36:44.72 +36:13:29.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 1.348 2048474554373077632 294.18616249943 +36.22507026173 13.7198 12.8617 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.348#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 328812_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 328812_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:45:54.17 +39:43:41.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 5.563 2073328464968326016 296.47474917453 +39.72678101548 14.0924 13.5189 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.563#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 328815_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 328815_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:32:10.65 +38:48:09.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)
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Considering the candidate 328825_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 328825_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:31:32.39 +38:20:47.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)
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Considering the candidate 328827_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 328827_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:01:30.77 +39:25:30.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)
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Considering the candidate 328829_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 328829_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 328832_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 328832_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:00:47.52 +33:10:07.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 3.184 2034205264292157952 300.19888526671 +33.16920484886 12.5862 11.6096 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.184#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 328839_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 328839_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:24:27.68 +40:28:49.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 3.602 2101499018012553984 291.11423772634 +40.48108158072 13.7976 13.2646 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.602#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 328843_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 328843_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 328844_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 328844_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:00:58.69 +39:20:39.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)
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Considering the candidate 328850_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 328850_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 328854_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 328854_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:17:21.69 +41:18:12.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.25, MAG_FAINT_SEARCH_LIMIT=14.23)GAIADR2_OUTPUT=# 5.107 2068577887530953984 304.33979314911 +41.30473854623 12.8465 12.4117 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.107#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 328857_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 328857_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:28:42.95 +36:37:11.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 3.563 2051490068091055744 292.17892276436 +36.61895502545 13.8326 13.1581 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.563#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 328858_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 328858_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:01:06.10 +42:39:29.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)
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Considering the candidate 328862_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 328862_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 328869_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 328869_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:04:30.58 +34:01:13.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)
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Considering the candidate 328870_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 328870_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:15:30.04 +41:16:29.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 3.656 2062623340571947776 303.87560971146 +41.27576495755 13.0082 12.2879 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.656#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 328871_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 328871_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:05:24.84 +37:22:39.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)
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Considering the candidate 328873_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 328873_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 328877_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 328877_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:51:54.04 +42:31:40.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)
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Considering the candidate 328879_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 328879_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:11:04.68 +35:17:19.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 1.617 2058871188428174976 302.76895327292 +35.28888345075 12.8315 12.4216 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.617#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 328883_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 328883_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:32:15.74 +36:56:10.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)
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Considering the candidate 328890_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 328890_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:15:20.44 +39:11:54.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)
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Considering the candidate 328891_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 328891_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:10:55.84 +37:30:42.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 4.417 2060806951687706752 302.73273998815 +37.51044106374 13.0631 12.7369 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.417#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 328892_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 328892_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 328893_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 328893_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:55:03.76 +42:17:31.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 328894_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 328894_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 328895_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 328895_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 328896_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 328896_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:38:45.25 +37:08:56.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)
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Considering the candidate 328897_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 328897_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 328898_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 328898_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:07:42.10 +34:41:57.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 2.858 2058779830192001792 301.92451441761 +34.69899515553 12.5960 12.2092 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.858#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 328900_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 328900_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 328906_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 328906_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 328908_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 328908_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:36:02.46 +35:17:13.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)
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Considering the candidate 328911_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 328911_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:45:46.81 +37:16:30.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)
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Considering the candidate 328912_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 328912_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:17:53.38 +38:19:26.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 1.653 2061267677091003008 304.47294640747 +38.32380475964 12.6581 12.1536 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.653#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 328916_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 328916_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 328919_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 328919_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:57:22.64 +35:31:19.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)
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Considering the candidate 328923_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 328923_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:20:37.79 +33:26:59.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)
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Considering the candidate 328927_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 328927_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:42:57.40 +37:46:58.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)
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Considering the candidate 328935_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 328935_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 328944_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 328944_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 328946_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 328946_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:41:53.52 +35:18:52.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 2.308 2047427716239065216 295.47276861256 +35.31505723127 13.2283 12.8648 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.308#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 328947_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 328947_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:14:24.46 +34:47:58.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 3.832 2055831794688647680 303.60081461851 +34.80008828484 12.6570 12.1629 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.832#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 328948_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 328948_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 328953_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 328953_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 328954_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 328954_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 328955_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 328955_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:10.90 +34:52:51.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 4.313 2055842725392691200 303.29484480297 +34.88210234009 12.7044 11.6784 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.313#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 328956_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 328956_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 328958_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 328958_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:57:47.90 +33:10:20.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)
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Considering the candidate 328960_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 328960_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:15:32.76 +34:10:02.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.00, MAG_FAINT_SEARCH_LIMIT=13.98)GAIADR2_OUTPUT=# 5.092 2049500742316475904 288.88816425127 +34.16689871656 13.2381 12.5233 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.092#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 328963_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 328963_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 328964_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 328964_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 328965_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 328965_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 328968_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 328968_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 328970_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 328970_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:39:17.43 +36:12:30.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 2.222 2048650819835188864 294.82190678010 +36.20876818832 12.8392 12.0084 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.222#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 328972_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 328972_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:48:55.28 +37:33:45.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)
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Considering the candidate 328973_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 328973_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 328974_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 328974_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:10:15.96 +36:54:11.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)
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Considering the candidate 328975_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 328975_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 328977_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 328977_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 328980_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 328980_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:09:51.10 +34:12:48.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 4.260 2055704732371598208 302.46305846623 +34.21476094988 12.2750 11.7461 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.260#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 328981_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 328981_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:10:38.73 +35:48:16.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 5.483 2058947024691078016 302.66311068736 +35.80411319224 12.4619 11.3723 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.483#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 328982_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 328982_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 328983_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 328983_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:42:15.68 +39:16:27.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)
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Considering the candidate 328985_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 328985_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:25:37.52 +34:05:36.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)
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Considering the candidate 328987_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 328987_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:38.14 +36:14:42.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)
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Considering the candidate 328990_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 328990_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 328992_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 328992_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:09:23.16 +36:19:01.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 2.850 2059163697197936256 302.34737769451 +36.31738330797 12.3002 10.8268 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.850#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 328994_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 328994_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 328996_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 328996_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:15:20.35 +36:29:02.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 4.150 2060456070028454784 303.83394505763 +36.48318089248 12.3805 11.8254 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.150#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 328997_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 328997_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:45:14.80 +35:25:50.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)
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Considering the candidate 329000_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329000_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:14:52.90 +36:58:18.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 5.160 2060533929198631040 303.71955171689 +36.97311701539 12.7006 12.1677 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.160#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 329001_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 329001_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 329004_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329004_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:53:52.65 +35:20:33.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.75, MAG_FAINT_SEARCH_LIMIT=13.73)
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Considering the candidate 329006_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 329006_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 329007_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329007_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:54.65 +37:22:52.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 5.828 2060743798485677568 303.47588841781 +37.38186656444 12.7202 12.2415 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.828#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 329011_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329011_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:52:11.44 +37:46:16.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 2.861 2072110687130832640 298.04748487308 +37.77035713155 13.2880 12.5046 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.861#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 329012_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329012_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:59:38.85 +39:02:21.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)
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Considering the candidate 329014_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 329014_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 329018_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329018_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 329021_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 329021_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 329022_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329022_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:08:58.06 +33:18:14.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)
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Considering the candidate 329024_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329024_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:03:10.80 +39:40:04.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)
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Considering the candidate 329026_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329026_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:03:23.25 +33:41:59.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.58, MAG_FAINT_SEARCH_LIMIT=13.56)
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Considering the candidate 329029_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 329029_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 329034_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 329034_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 329038_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329038_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:58:55.86 +34:21:12.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 5.258 2058522849396890112 299.73235976730 +34.35475793675 12.7312 12.2370 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.258#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 329039_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329039_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:12:21.72 +33:58:37.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 0.446 2055639109587743872 303.09056330674 +33.97705671524 12.4035 11.3965 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.446#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 329041_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329041_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:45:40.33 +33:06:41.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)
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Considering the candidate 329043_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329043_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:15:09.01 +38:16:29.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)
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Considering the candidate 329044_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329044_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 329048_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329048_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:52:49.59 +34:36:41.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)
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Considering the candidate 329049_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329049_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 329052_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329052_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:02:47.77 +40:48:56.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)
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Considering the candidate 329053_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329053_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:21.08 +34:22:37.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 4.247 2055677966139531648 303.33687319798 +34.37787409703 12.0593 11.4177 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.247#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 329054_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 329054_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 329056_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 329056_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 329058_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329058_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:02:30.42 +39:24:29.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 4.427 2073992290805043712 300.62583963716 +39.40917523598 12.5254 11.2783 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.427#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 329059_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329059_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:09:11.46 +34:55:52.2 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 329060_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329060_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
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Considering the candidate 329061_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 329061_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 329062_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 329062_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 329063_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329063_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:47:41.87 +36:47:21.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 5.320 2047989154364106880 296.92338112336 +36.79047753480 12.0291 10.5329 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.320#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 329067_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329067_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:12.65 +34:06:52.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 4.258 2055653467644816896 303.30372598980 +34.11535778079 12.3369 11.9011 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.258#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 329068_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329068_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:51:22.65 +39:06:32.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 0.643 2073368627192642048 297.84414639713 +39.10915888711 12.4168 11.9573 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.643#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 329072_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329072_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 329074_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 329074_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 329076_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329076_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:06:29.84 +34:10:05.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 1.387 2058320676695417856 301.62387001258 +34.16817716592 12.2058 11.0427 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.387#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 329077_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329077_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:12:42.02 +34:57:40.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 1.533 2055845817769274240 303.17533143866 +34.96151312088 12.0080 11.0068 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.533#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 329080_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329080_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:59:14.80 +36:43:16.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 3.946 2059809729010728320 299.81145252503 +36.72238816551 11.9211 10.7701 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.946#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 329081_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329081_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:49:58.10 +36:32:39.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)
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Considering the candidate 329082_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329082_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:53:46.74 +33:50:01.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.98, MAG_FAINT_SEARCH_LIMIT=12.96)GAIADR2_OUTPUT=# 3.999 2035134282901593728 298.44589897875 +33.83437410094 11.9110 10.6290 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.999#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 329083_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329083_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:17:34.76 +33:59:45.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.00, MAG_FAINT_SEARCH_LIMIT=12.98)GAIADR2_OUTPUT=# 3.098 2049457032425494400 289.39471931865 +33.99685548577 11.3908 9.7917 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.098#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 329084_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 329084_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 329085_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329085_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:59.53 +37:25:38.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.57, MAG_FAINT_SEARCH_LIMIT=12.55)
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Considering the candidate 329086_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329086_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:15:30.84 +35:36:38.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 329087_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329087_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:10:18.80 +35:09:37.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 329088_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329088_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:10:37.85 +33:10:58.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 329106_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329106_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:19:20.81 +41:23:30.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 329134_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329134_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:12:10.48 +33:13:50.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 329181_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329181_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:12:22.81 +32:52:17.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 329182_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329182_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:18:45.14 +39:24:22.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 329186_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329186_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:45.74 +33:37:19.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 329204_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329204_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:28.20 +33:22:53.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 329208_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329208_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:11:57.77 +33:00:43.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 329230_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329230_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:09.86 +33:27:27.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 329253_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329253_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:12:11.96 +33:03:34.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 329269_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329269_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:41.21 +33:18:46.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 329336_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329336_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:12:28.34 +33:22:22.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 329432_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329432_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:19.80 +33:00:35.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 329458_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329458_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:09.16 +33:09:13.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 329461_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329461_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:12:44.56 +33:03:00.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 329497_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329497_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:12:26.03 +33:09:37.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 329614_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329614_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:17.53 +33:06:24.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 329736_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329736_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:12:29.85 +32:52:11.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 329750_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329750_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:12:57.26 +33:06:35.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 329836_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329836_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:14:07.30 +33:48:57.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 329859_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329859_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:26.04 +33:34:16.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 329865_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329865_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:12:33.82 +33:11:53.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 329870_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329870_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:31.10 +33:49:53.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 329940_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 329940_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:01.29 +32:58:28.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 330058_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 330058_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:03.75 +33:01:30.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 330070_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 330070_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:05.56 +32:57:06.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 330140_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 330140_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:12.14 +32:50:38.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.59, MAG_FAINT_SEARCH_LIMIT=12.57)GAIADR2_OUTPUT=# 1.423 2054965005862252672 303.30018441094 +32.84415389616 11.3615 10.4923 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.423#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 330143_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 330143_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:14:08.09 +34:05:52.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.45, MAG_FAINT_SEARCH_LIMIT=12.43)GAIADR2_OUTPUT=# 4.605 2055656083299318912 303.53520964881 +34.09764379816 10.7986 9.5972 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.605#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 330195_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 330195_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:12:18.52 +32:59:42.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.46, MAG_FAINT_SEARCH_LIMIT=12.44)GAIADR2_OUTPUT=# 4.432 2055017404474777984 303.07693326974 +32.99624329899 11.2663 10.9109 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.432#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 330259_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 330259_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:06:12.90 +32:49:52.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.55, MAG_FAINT_SEARCH_LIMIT=12.53)GAIADR2_OUTPUT=# 3.296 2055131925496534016 301.55481995668 +32.83104966510 10.8933 9.5475 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.296#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 330287_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 330287_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:11:52.14 +33:15:39.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.52, MAG_FAINT_SEARCH_LIMIT=12.50)GAIADR2_OUTPUT=# 3.667 2055044441281102208 302.96816708146 +33.26175368974 11.0443 9.8538 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.667#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 330288_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 330288_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:12:40.66 +32:58:38.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.54, MAG_FAINT_SEARCH_LIMIT=12.52)GAIADR2_OUTPUT=# 4.151 2055016682920195072 303.16931112853 +32.97839957993 11.2940 10.8157 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.151#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 330314_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 330314_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 330345_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 330345_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:12:58.90 +33:26:28.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.64, MAG_FAINT_SEARCH_LIMIT=12.62)GAIADR2_OUTPUT=# 3.148 2055419172902465152 303.24499504869 +33.44196735674 11.3099 10.4510 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.148#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 330351_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 330351_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:44.03 +33:49:12.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.60, MAG_FAINT_SEARCH_LIMIT=12.58)GAIADR2_OUTPUT=# 4.597 2055435459407562112 303.43426765465 +33.82111336104 11.1406 10.0730 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.597#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 330405_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 330405_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:12:59.90 +33:44:18.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.65, MAG_FAINT_SEARCH_LIMIT=12.63)GAIADR2_OUTPUT=# 2.630 2055620727127078016 303.25021736891 +33.73903354067 11.2743 10.3004 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.630#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 330410_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 330410_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:10.10 +33:07:42.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.62, MAG_FAINT_SEARCH_LIMIT=12.60)GAIADR2_OUTPUT=# 2.688 2055025096748410880 303.29236147331 +33.12904282311 11.1386 10.1514 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.688#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 330472_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 330472_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:12:40.48 +32:48:16.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.66, MAG_FAINT_SEARCH_LIMIT=12.64)GAIADR2_OUTPUT=# 2.424 2054966105384219392 303.16944376867 +32.80469116977 11.2154 10.2317 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.424#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 330501_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 330501_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:12:58.20 +32:50:35.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.78, MAG_FAINT_SEARCH_LIMIT=12.76)GAIADR2_OUTPUT=# 3.400 2054967647265881984 303.24192028900 +32.84400366413 11.7085 11.2460 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.400#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 330605_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 330605_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:12:34.70 +33:01:38.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.78, MAG_FAINT_SEARCH_LIMIT=12.76)GAIADR2_OUTPUT=# 5.335 2055017679352653184 303.14446970513 +33.02895122401 11.5231 11.1745 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.335#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 330626_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 330626_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:31.77 +33:10:04.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.84, MAG_FAINT_SEARCH_LIMIT=12.82)GAIADR2_OUTPUT=# 3.920 2055025410293687808 303.38258666171 +33.16893536498 11.5511 10.5453 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.920#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 330679_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 330679_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:12:52.35 +33:05:58.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.85, MAG_FAINT_SEARCH_LIMIT=12.83)GAIADR2_OUTPUT=# 3.255 2055024173343645696 303.21875283293 +33.10020780384 11.4206 10.3649 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.255#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 330691_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 330691_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:01:41.76 +33:36:12.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 330713_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 330713_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:16:01.68 +34:38:03.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 2.377 2049551384270392192 289.00651726498 +34.63472199902 12.4358 10.6692 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.377#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 330741_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 330741_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:47:47.64 +32:48:00.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.97, MAG_FAINT_SEARCH_LIMIT=12.95)GAIADR2_OUTPUT=# 5.210 2034733339119504640 296.94942556158 +32.80144265224 12.3587 11.2300 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.210#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 330749_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 330749_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:12:38.06 +32:49:53.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.87, MAG_FAINT_SEARCH_LIMIT=12.85)GAIADR2_OUTPUT=# 2.819 2054967028790592384 303.15817091101 +32.83209115761 11.6234 11.1943 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#
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Considering the candidate 330785_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 330785_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:19:10.28 +40:47:52.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 3.048 2068350627917870592 304.79220673865 +40.79853478518 11.9827 11.5589 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.048#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 330822_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 330822_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:12:43.07 +33:05:44.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.96, MAG_FAINT_SEARCH_LIMIT=12.94)GAIADR2_OUTPUT=# 4.251 2055024035904261760 303.17926054894 +33.09691918831 11.7382 11.1981 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.251#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 330847_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 330847_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 330860_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 330860_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:31.55 +33:17:04.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.99, MAG_FAINT_SEARCH_LIMIT=12.97)GAIADR2_OUTPUT=# 3.311 2055402611508355584 303.38118206456 +33.28550131481 11.7597 10.9071 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.311#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 330869_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 330869_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:12:40.44 +32:51:31.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.93, MAG_FAINT_SEARCH_LIMIT=12.91)GAIADR2_OUTPUT=# 1.992 2054968609338554368 303.16886084665 +32.85921279617 11.5958 10.7917 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.992#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 330882_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 330882_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:32.10 +33:24:07.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.99, MAG_FAINT_SEARCH_LIMIT=12.97)GAIADR2_OUTPUT=# 3.289 2055407731109442304 303.38405522920 +33.40307190029 11.6331 10.7509 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.289#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 330909_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 330909_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 330949_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 330949_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 330974_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 330974_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:12:39.03 +33:56:35.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 1.545 2055628526788289408 303.16313994555 +33.94304096260 12.0166 11.1651 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.545#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 330989_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 330989_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:14:09.82 +34:11:45.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 1.061 2055660721864090112 303.54126827546 +34.19584153487 11.9021 11.4227 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.061#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 330998_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 330998_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:12:02.93 +33:03:02.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 4.930 2055021424564259456 303.01185298917 +33.05194765998 12.1729 11.6771 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.930#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 331018_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 331018_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:54:18.10 +34:31:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 2.772 2035332401149328256 298.57582196316 +34.53299924873 11.0363 9.5567 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.772#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 331029_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 331029_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 331053_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 331053_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:12:01.22 +33:13:03.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 3.604 2055041147054198784 303.00616113691 +33.21799053740 11.4620 10.2771 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.604#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 331106_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 331106_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:39.88 +33:27:01.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 4.220 2055409036779504256 303.41572931395 +33.45144722539 11.8780 11.3229 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.220#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 331108_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 331108_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:58.22 +33:46:56.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 5.362 2055454872672590976 303.49238377822 +33.78381360141 11.8667 11.4544 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.362#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 331121_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 331121_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:43:13.63 +40:01:18.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 0.996 2076373493698033152 295.80714984196 +40.02171317770 12.0550 11.1102 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.996#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 331231_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 331231_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:11:50.40 +33:01:02.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.16, MAG_FAINT_SEARCH_LIMIT=13.14)GAIADR2_OUTPUT=# 3.520 2055019775296844032 302.95957219574 +33.01815967051 12.0576 11.6505 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.520#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 331232_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 331232_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:08:44.72 +32:49:20.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 4.599 2055099519958526592 302.18728635746 +32.82335643251 12.2982 11.7882 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.599#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 331234_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 331234_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:13:28.06 +39:01:05.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 2.465 2099676096450847616 288.36682201243 +39.01876402929 12.6036 11.9097 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.465#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 331252_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 331252_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:12:58.25 +33:05:33.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 3.792 2055024203395216256 303.24286384843 +33.09362855290 11.9975 11.5470 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.792#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 331365_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 331365_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:06:08.29 +41:25:19.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 331398_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 331398_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:10:46.57 +32:50:10.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 1.029 2055004927582011392 302.69434912510 +32.83631647624 11.7825 10.8528 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.029#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 331440_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 331440_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:11:13.61 +40:25:16.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 331442_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 331442_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:12:02.37 +32:57:22.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 3.440 2055018602757872640 303.00984673601 +32.95726089112 11.8492 11.2922 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.440#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 331465_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 331465_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 331511_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 331511_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 331549_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 331549_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:14:09.04 +34:12:20.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.33, MAG_FAINT_SEARCH_LIMIT=13.31)GAIADR2_OUTPUT=# 2.510 2055660721864107136 303.53850796327 +34.20573481574 11.8189 10.7266 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.510#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 331564_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 331564_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:40:51.71 +43:05:19.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 331590_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 331590_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 331621_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 331621_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:58:46.58 +35:30:42.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.48, MAG_FAINT_SEARCH_LIMIT=13.46)GAIADR2_OUTPUT=# 4.717 2059405860309203456 299.69256186858 +35.51209426693 12.5847 12.0483 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.717#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 331642_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 331642_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:56:44.09 +37:37:35.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 3.950 2072289667014514944 299.18384558244 +37.62764742331 13.4170 11.3765 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.950#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 331818_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 331818_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 331821_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 331821_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:56.49 +33:48:08.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 5.026 2055457930689334400 303.48625819521 +33.80349309840 12.2433 11.3081 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.026#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 331830_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 331830_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:20.63 +33:31:50.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 3.974 2055421475004914688 303.33602752306 +33.53168567553 12.8853 12.1171 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.974#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 331842_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 331842_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:13.45 +33:16:17.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)
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Considering the candidate 331860_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 331860_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:11:41.70 +33:00:38.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.49, MAG_FAINT_SEARCH_LIMIT=13.47)GAIADR2_OUTPUT=# 4.961 2055020015815460480 302.92408422846 +33.01215479775 12.2757 11.7656 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.961#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 331871_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 331871_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:05:17.88 +33:28:37.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 3.086 2058194512063799680 301.32476454007 +33.47625513807 11.0551 9.5992 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.086#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 331886_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 331886_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:12:25.74 +33:03:24.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.50, MAG_FAINT_SEARCH_LIMIT=13.48)GAIADR2_OUTPUT=# 4.322 2055020977887581312 303.10686025520 +33.05784977705 12.2321 11.7503 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.322#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 331887_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 331887_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:08.64 +33:03:23.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 5.151 2055023108191225984 303.28511757460 +33.05769704512 11.9151 11.5998 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.151#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 331893_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 331893_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:02:52.23 +38:30:07.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 3.397 2100020174870740480 285.71754060514 +38.50305253466 12.8663 12.0310 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.397#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 331903_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 331903_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:05.01 +34:22:37.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 1.844 2055678825143784576 303.27049999568 +34.37659180127 12.3117 11.4370 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.844#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 331927_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 331927_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:47:48.83 +42:19:48.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 331930_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 331930_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:30.10 +33:21:52.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.49, MAG_FAINT_SEARCH_LIMIT=13.47)GAIADR2_OUTPUT=# 2.947 2055407524950994560 303.37629788536 +33.36488626781 12.1703 11.1029 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.947#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 331935_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 331935_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:08:03.85 +32:51:25.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)
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Considering the candidate 331958_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 331958_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:12:16.63 +33:04:43.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 1.428 2055021149686319616 303.06886529737 +33.07886702945 12.2442 11.6262 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.428#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 331981_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 331981_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:33:27.97 +38:31:57.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 2.752 2052287145299902848 293.36712885317 +38.53336118544 13.2487 11.3950 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.752#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 332022_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 332022_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:16:35.22 +38:07:57.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 332099_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 332099_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:30.95 +33:41:15.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 5.042 2055432160884072832 303.37961746282 +33.68898318759 12.2538 11.3645 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.042#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 332165_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 332165_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:02.70 +33:29:53.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 4.045 2055421646803647488 303.26139467272 +33.49939497984 12.2713 11.3743 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.045#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 332197_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 332197_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 332230_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 332230_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:11:26.88 +32:48:32.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 3.997 2054993833693741952 302.86188315578 +32.80999478441 12.4199 11.8915 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.997#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 332239_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 332239_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:16.82 +33:08:39.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.75, MAG_FAINT_SEARCH_LIMIT=13.73)GAIADR2_OUTPUT=# 3.395 2055025513372932352 303.32073485015 +33.14510260276 12.6148 12.0824 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.395#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 332266_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 332266_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:12:50.37 +32:48:08.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 4.115 2054965963638706944 303.21120971197 +32.80252506649 12.0855 10.9938 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.115#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 332299_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 332299_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:14.00 +32:59:51.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)
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Considering the candidate 332304_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 332304_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:12:46.82 +32:55:38.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 4.364 2054969438278539264 303.19567181805 +32.92832937713 12.1600 11.0502 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.364#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 332311_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 332311_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:39:03.75 +34:58:00.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)
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Considering the candidate 332334_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 332334_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:12:52.38 +34:15:05.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 2.567 2055671197271076224 303.21900943998 +34.25113406478 12.1268 10.8599 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.567#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 332336_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 332336_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 332350_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 332350_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:12:13.32 +33:24:12.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)GAIADR2_OUTPUT=# 3.401 2055047052621209856 303.05538803840 +33.40438445716 12.0264 11.4480 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.401#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 332411_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 332411_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 332459_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 332459_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:01.54 +33:38:10.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 3.379 2055426663325525120 303.25665575765 +33.63719511508 12.1773 11.2852 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.379#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 332461_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 332461_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:12:14.47 +33:08:26.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 2.839 2055028193432733312 303.06119536669 +33.14077736517 11.7178 10.0845 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.839#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 332485_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 332485_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 332507_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 332507_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:12:10.89 +32:53:58.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 5.019 2055015274171527552 303.04556891326 +32.90107914821 12.3164 11.4548 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.019#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 332518_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 332518_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:32:50.91 +39:40:08.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 4.216 2053225853350045184 293.21224960892 +39.67011167200 13.0662 12.2256 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.216#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 332522_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 332522_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 332556_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 332556_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:32.35 +33:06:13.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 4.782 2054978200011778176 303.38494466311 +33.10504423114 12.6158 12.0768 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.782#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 332576_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 332576_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:02:05.99 +33:37:47.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 0.128 2058246322217374592 300.52499836155 +33.62992916562 12.4188 11.1215 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.128#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 332578_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 332578_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:43:52.36 +33:54:56.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 332583_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 332583_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:05.87 +33:38:10.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 3.023 2055431778609910016 303.27491864935 +33.63702488386 12.6869 11.7712 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.023#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 332587_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 332587_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:14.10 +33:00:59.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 3.336 2054975790523861632 303.30962255451 +33.01720773330 12.1258 10.8568 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.336#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 332616_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 332616_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:12:56.75 +33:39:17.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.75, MAG_FAINT_SEARCH_LIMIT=13.73)GAIADR2_OUTPUT=# 2.087 2055426732045026560 303.23681705111 +33.65544146011 12.3825 11.4822 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 332628_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 332628_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:16:48.64 +38:13:06.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 5.509 2061260328424590208 304.20460278632 +38.21872211018 12.6249 10.5691 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.509#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 332638_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 332638_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:12:47.79 +33:19:06.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)GAIADR2_OUTPUT=# 5.862 2055042899400747520 303.19948180853 +33.31996178976 12.3923 11.5544 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.862#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 332688_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 332688_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:12:13.61 +33:02:12.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 4.204 2055020664342169344 303.05587654082 +33.03785341813 12.6509 12.1694 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.204#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 332694_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 332694_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 332727_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 332727_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:57:05.92 +32:49:56.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 0.544 2034269791893011328 299.27459957435 +32.83239030685 12.6169 11.6676 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.544#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 332761_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 332761_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:12:36.78 +33:00:09.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.75, MAG_FAINT_SEARCH_LIMIT=13.73)GAIADR2_OUTPUT=# 5.821 2055017606325456384 303.15368927700 +33.00424111557 12.3313 11.4323 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.821#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 332767_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 332767_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:44.62 +34:13:35.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 0.730 2055661542186031488 303.43615120074 +34.22655181909 12.5585 11.6281 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.730#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 332784_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 332784_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:12:36.63 +33:44:23.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 1.145 2055615843727346560 303.15268643215 +33.74011948778 12.3285 11.4093 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.145#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 332894_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 332894_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:12:36.83 +33:03:36.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 2.437 2055023795386092160 303.15388371463 +33.06076999792 12.3856 11.4881 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.437#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 332908_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 332908_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:07:25.26 +38:28:43.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 332916_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 332916_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 332917_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 332917_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:11:02.33 +33:02:32.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.83, MAG_FAINT_SEARCH_LIMIT=13.81)GAIADR2_OUTPUT=# 1.310 2055012005688100224 302.75955483891 +33.04281265133 12.4929 11.4915 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.310#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 332936_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 332936_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 332945_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 332945_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:11:45.48 +32:50:04.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 3.196 2054991359792688512 302.94055008892 +32.83454361042 12.2336 11.1347 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.196#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 332950_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 332950_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 332955_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 332955_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:04.53 +33:10:41.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 3.449 2055026230619774080 303.26803276784 +33.17892660713 12.4975 11.6168 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.449#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 332966_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 332966_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:14:22.35 +34:05:16.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 4.102 2055655872826503424 303.59196731320 +34.08738442268 12.6584 11.9853 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.102#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 332974_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 332974_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:03:22.55 +33:20:59.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 2.065 2058177538351572608 300.84431132345 +33.35040881178 11.8363 10.1036 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.065#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 333014_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 333014_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:07:52.93 +38:56:08.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 4.398 2100370575481932032 286.97177524282 +38.93642298152 13.5387 12.8043 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.398#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 333039_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 333039_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:40:40.63 +36:06:55.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 4.583 2048599692542391808 295.16910779396 +36.11676441472 11.7732 10.1579 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.583#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 333052_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 333052_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:12:06.54 +33:23:50.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 3.779 2055047086993401600 303.02762116554 +33.39822527633 12.3448 11.4573 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.779#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 333073_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 333073_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:37.91 +33:16:48.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 4.565 2055402508429116160 303.40810713565 +33.28134535269 12.7831 12.0156 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.565#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 333074_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 333074_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 333176_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 333176_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:41:46.73 +33:13:39.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 3.896 2046902626403065984 295.44532002780 +33.22850916863 12.2209 10.6945 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.896#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 333199_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 333199_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:15:37.04 +37:35:41.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 3.837 2060834813114021632 303.90453938368 +37.59585892234 12.4852 11.0374 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.837#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 333238_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 333238_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:06:00.39 +32:49:51.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 2.056 2055131788057634560 301.50139095274 +32.83148069517 12.5461 11.6784 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.056#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 333242_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 333242_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:52:10.12 +40:47:32.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 5.032 2073798128229217664 298.04353085973 +40.79341428250 13.1495 12.2825 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.032#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 333283_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 333283_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:53.36 +34:01:48.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)
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Considering the candidate 333288_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 333288_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:12.16 +33:22:57.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)
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Considering the candidate 333299_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 333299_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 333418_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 333418_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:44:52.80 +42:02:02.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 333455_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 333455_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:02.22 +36:51:34.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 5.280 2060694316138043392 303.26068005391 +36.86036192635 12.3069 10.7115 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.280#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 333473_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 333473_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:10:40.59 +42:01:23.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 4.846 2102404053519321472 287.67006176671 +42.02429119196 13.7887 13.3626 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.846#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 333488_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 333488_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 333511_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 333511_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:30.39 +33:47:48.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)
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Considering the candidate 333538_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 333538_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:12:38.59 +33:40:26.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 5.120 2055614778575372800 303.16237869354 +33.67461059829 11.8994 10.3942 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.120#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 333556_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 333556_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:12:01.63 +33:19:33.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 5.634 2055045167143854464 303.00804432968 +33.32699692016 12.7464 11.5846 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.634#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 333569_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 333569_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:49:09.83 +36:39:30.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 4.633 2071955445509790720 297.29088495353 +36.65975770989 11.5613 9.8501 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.633#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 333615_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 333615_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:09.96 +33:13:15.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)
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Considering the candidate 333617_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 333617_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 333632_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 333632_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:44:06.42 +37:21:38.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 333675_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 333675_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 333752_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 333752_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 333774_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 333774_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:12:30.64 +33:33:18.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 4.849 2055424601741271296 303.12900904504 +33.55580591352 12.8778 11.6064 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.849#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 333812_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 333812_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:01:55.07 +38:56:29.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 2.574 2072427617033694976 300.47974050910 +38.94220828954 13.2009 12.3277 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.574#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 333832_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 333832_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 333912_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 333912_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:11:26.49 +33:19:57.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 3.592 2055227647402744704 302.86149806770 +33.33292285579 12.7123 11.4769 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.592#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 333947_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 333947_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:49:34.42 +32:48:17.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 2.531 2034724027629545088 297.39313633858 +32.80538473662 12.8523 12.3856 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.531#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 333981_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 333981_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:10:18.18 +32:53:02.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.17, MAG_FAINT_SEARCH_LIMIT=14.15)GAIADR2_OUTPUT=# 0.761 2055003385701076352 302.57596426351 +32.88422193959 12.8371 11.8795 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.761#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 334015_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 334015_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:12:39.26 +33:20:04.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 4.850 2055043071199484160 303.16435111383 +33.33585142993 12.6223 11.5929 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.850#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 334028_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 334028_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:07:36.79 +39:56:31.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 334030_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 334030_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:36:15.00 +33:04:19.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 1.576 2045629533685835008 294.06225258149 +33.07252456320 13.8917 12.0365 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.576#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 334032_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 334032_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:11:16.31 +33:07:34.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 0.812 2055036229303642752 302.81812479983 +33.12653849815 12.7057 11.6121 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.812#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 334036_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 334036_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:12:36.45 +33:53:50.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 3.300 2055626740081480448 303.15212643682 +33.89822591796 12.7844 11.6584 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.300#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 334071_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 334071_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:02:33.64 +42:30:44.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 3.329 2104210929080250624 285.63958354551 +42.51304093208 13.5992 12.9201 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.329#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 334089_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 334089_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 334105_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 334105_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:23:47.31 +40:48:09.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 5.354 2101524341140348800 290.94734618097 +40.80411661474 14.1330 13.5697 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.354#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 334185_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 334185_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:56:26.72 +39:58:34.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 3.903 2073525135798784384 299.11274813874 +39.97629561522 13.9262 11.4362 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.903#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 334200_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 334200_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:03:21.28 +40:08:26.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 5.163 2100725649018526592 285.83855918898 +40.14220964923 13.8136 13.2954 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.163#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 334221_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 334221_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:04.20 +32:52:45.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 5.183 2054968093942687872 303.26916909174 +32.87957866170 12.2440 10.7479 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.183#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 334249_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 334249_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:38:01.35 +33:11:12.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 2.802 2045465186747487872 294.50572966769 +33.18760674796 13.0252 11.6362 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.802#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 334330_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 334330_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:35.97 +33:39:05.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 3.610 2055429102867318400 303.40080421783 +33.65208241132 12.7589 11.4986 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.610#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 334352_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 334352_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:12:18.53 +37:00:53.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.50, MAG_FAINT_SEARCH_LIMIT=14.48)GAIADR2_OUTPUT=# 5.605 2060711431609605248 303.07847914577 +37.01595882300 12.1544 10.5328 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.605#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 334372_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 334372_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:54:27.52 +42:04:16.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 334462_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 334462_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:06:27.70 +37:41:21.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 4.665 2060108590011878144 301.61582347596 +37.69067195762 12.2938 10.6570 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.665#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 334566_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 334566_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:52.98 +33:55:58.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)
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Considering the candidate 334591_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 334591_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:04:13.01 +35:07:06.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 3.021 2058675612789760000 301.05498674835 +35.11899092420 12.3969 10.7358 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.021#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 334605_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 334605_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:16:28.26 +41:50:02.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.06, MAG_FAINT_SEARCH_LIMIT=15.04)GAIADR2_OUTPUT=# 2.995 2102254038902605696 289.11728405469 +41.83464507304 12.9477 11.4072 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.995#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 334610_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 334610_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:01:04.24 +36:49:28.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 3.458 2060130133574529408 300.26770169164 +36.82565472125 12.3401 10.7024 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.458#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 334624_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 334624_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 334743_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 334743_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:13:11.64 +38:31:43.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.75, MAG_FAINT_SEARCH_LIMIT=14.73)GAIADR2_OUTPUT=# 5.833 2061705007849483520 303.29952118747 +38.53027090635 12.3770 10.7879 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.833#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 334820_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 334820_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:47:26.23 +34:33:46.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)GAIADR2_OUTPUT=# 1.169 2047462763176733184 296.85932057263 +34.56310168693 13.1923 11.8249 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.169#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 334881_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 334881_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 334917_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 334917_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:50:51.61 +35:33:05.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 1.823 2047631125894146432 297.71468050228 +35.55205138972 12.6343 11.0570 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.823#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 334995_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 334995_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:51:48.91 +34:26:28.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 2.408 2035503993680072832 297.95386113056 +34.44188856220 13.0507 11.6595 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.408#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 334998_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 334998_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:06:02.30 +34:06:52.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 1.607 2058365486104893952 301.50940293673 +34.11427375301 12.5964 11.0565 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.607#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 335063_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 335063_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:38:52.84 +34:02:28.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 4.036 2047196921872583040 294.72045080471 +34.04237384221 13.1677 11.7489 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.036#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 335159_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 335159_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:52:17.85 +35:53:54.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 4.603 2071661296117084416 298.07481386429 +35.89961715522 12.6442 11.1239 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.603#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 335175_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 335175_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:52:46.04 +35:44:07.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 3.765 2059646795130792192 298.19188541020 +35.73657274011 14.4117 12.6289 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.765#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 335186_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 335186_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:49:44.87 +34:30:08.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 2.494 2035458600141760640 297.43704699198 +34.50305012028 12.8976 11.4662 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.494#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 335256_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 335256_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:47:21.01 +40:28:20.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)GAIADR2_OUTPUT=# 2.980 2076726402567711360 296.83718801760 +40.47306050726 13.5558 12.8457 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.980#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 209361_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 209361_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:13:46.06 +39:08:45.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 181120_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 181120_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:16:22.51 +38:08:01.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 29971_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 29971_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:46:25.63 +33:43:33.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 130322_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 130322_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:59:54.89 +37:02:35.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 56499_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 56499_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:31:46.52 +34:27:16.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 52283_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 52283_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:44:38.08 +34:24:55.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 175993_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 175993_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:55:51.38 +38:29:10.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 186268_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 186268_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:50:33.74 +38:43:24.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 159231_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 159231_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:50:46.59 +37:49:35.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 302732_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 302732_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:52:14.66 +37:19:29.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.37, MAG_FAINT_SEARCH_LIMIT=12.35)GAIADR2_OUTPUT=# 2.172 2072082683943265536 298.06083395753 +37.32543078633 11.1494 10.3459 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.172#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 172699_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 172699_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 73311_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 73311_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 39037_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 39037_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 04763_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 04763_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 153320_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 153320_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 305022_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 305022_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:11:55.20 +33:57:14.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 5.159 2055639521904326784 302.98045702305 +33.95532651229 12.5234 11.6796 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.159#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 126280_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 126280_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 18022_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 18022_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:05:49.34 +33:27:37.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)
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Considering the candidate 167637_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 167637_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 45702_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 45702_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:09:23.93 +34:23:42.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 4.894 2058710148640138752 302.35111779443 +34.39584293057 12.4301 11.6876 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.894#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 167956_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 167956_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 126901_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 126901_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 65325_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 65325_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 216463_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 216463_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 195579_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 195579_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 18255_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 18255_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 248978_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 248978_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 165990_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 165990_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 162928_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 162928_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 16491_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 16491_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 309785_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 309785_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:06:39.31 +33:52:39.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 40574_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 40574_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:43:09.17 +34:10:34.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 44553_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 44553_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 16502_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 16502_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 152505_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 152505_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 232967_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 232967_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:50:40.04 +40:43:07.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.92, MAG_FAINT_SEARCH_LIMIT=13.90)
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Considering the candidate 57394_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 57394_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 19288_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 19288_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 46295_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 46295_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 100017_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 100017_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 34500_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 34500_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 242512_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 242512_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:45:28.11 +41:17:26.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 230836_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 230836_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 119998_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 119998_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 201305_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 201305_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 301091_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 301091_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:53:36.70 +34:17:41.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 4.115 2035297079337067008 298.40424085055 +34.29439069233 12.9848 11.5262 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.115#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 65442_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 65442_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 14305_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 14305_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 301653_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 301653_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:13:17.69 +37:03:23.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.87, MAG_FAINT_SEARCH_LIMIT=11.85)
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Considering the candidate 160894_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 160894_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:11:45.63 +38:00:46.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 232006_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 232006_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:19:53.68 +40:15:21.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 288432_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 288432_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 22707_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 22707_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 289188_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 289188_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 111752_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 111752_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 143342_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 143342_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 302162_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 302162_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:00:57.73 +38:54:42.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 2.580 2072471769297500288 300.24084342285 +38.91251057577 12.9556 10.6504 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.580#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 302138_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 302138_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:23:05.52 +33:56:17.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)GAIADR2_OUTPUT=# 1.751 2049314370789636608 290.77300113653 +33.93873647102 12.5289 11.0425 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.751#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129865_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 129865_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:32:55.92 +36:50:28.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103957_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 103957_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 327062_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 327062_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:58:14.86 +35:43:19.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 2.423 2059693318219261568 299.56182201639 +35.72286318923 12.7143 11.3249 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.423#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 301619_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 301619_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:32:42.84 +34:20:54.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 5.889 2046571295439236352 293.17867662081 +34.35018478074 12.3420 11.2301 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.889#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 301615_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 301615_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 301595_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 301595_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:07:18.03 +34:44:50.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 1.966 2058408813737035520 301.82578764180 +34.74728964032 12.9971 12.4225 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.966#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 301347_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 301347_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:34:52.80 +35:38:59.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 4.244 2048339447579170048 293.72027900664 +35.65110146643 12.2231 10.6944 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.244#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 142657_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 142657_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 301179_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 301179_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:31:04.31 +37:33:13.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)
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Considering the candidate 203704_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 203704_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:55:13.27 +39:33:00.1 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 232332_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 232332_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:51:33.51 +40:39:37.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 44970_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 44970_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 107705_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 107705_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 105317_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 105317_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:10:31.51 +36:19:09.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 300916_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 300916_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:04:04.10 +38:24:26.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 2.292 2099969185019087488 286.01761921775 +38.40679921852 14.1483 13.6254 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.292#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 117143_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 117143_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:10:56.52 +36:34:46.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 207333_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 207333_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 20789_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 20789_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:41:28.04 +33:28:23.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)
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Considering the candidate 68151_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 68151_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 56758_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 56758_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 109436_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 109436_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:41:08.12 +36:24:39.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.86, MAG_FAINT_SEARCH_LIMIT=12.84)
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Considering the candidate 138528_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 138528_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 65542_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 65542_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 27959_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 27959_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 126758_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 126758_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 95139_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 95139_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 21315_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 21315_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 126056_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 126056_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 86038_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 86038_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 07635_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 07635_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 68699_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 68699_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:07:56.67 +34:29:11.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 111548_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 111548_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:15:41.77 +36:28:27.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)
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Considering the candidate 19198_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 19198_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 20497_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 20497_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 170301_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 170301_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 29483_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 29483_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 237125_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 237125_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 35666_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 35666_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 119295_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 119295_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 135087_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 135087_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 51578_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 51578_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 34341_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 34341_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 112623_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 112623_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 38894_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 38894_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 175381_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 175381_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 73977_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 73977_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 29364_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 29364_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 118307_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 118307_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 138696_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 138696_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 120666_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 120666_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 129076_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 129076_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 60354_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 60354_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 95909_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 95909_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 73680_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 73680_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 87654_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 87654_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 227622_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 227622_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 101733_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 101733_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:35:21.64 +36:03:60.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 97337_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 97337_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 79858_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 79858_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 260830_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 260830_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:48:26.70 +42:47:32.7 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 79539_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 79539_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 148202_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 148202_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 38391_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 38391_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 114759_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 114759_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 60677_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 60677_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 87981_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 87981_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 158551_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 158551_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 121038_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 121038_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 55805_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 55805_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:56:53.49 +34:44:54.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 46877_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 46877_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 14293_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 14293_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:54:46.06 +33:17:59.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 49728_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 49728_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 133806_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 133806_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 85005_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 85005_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 143467_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 143467_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 140668_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 140668_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 222848_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 222848_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 204948_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 204948_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 18399_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 18399_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 103529_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 103529_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 61065_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 61065_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:31:31.36 +34:42:16.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 15841_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 15841_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 120170_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 120170_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 39079_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 39079_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 81833_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 81833_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 182265_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 182265_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:07:15.90 +38:09:26.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)
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Considering the candidate 04799_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 04799_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 30235_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 30235_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 231829_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 231829_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 55729_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 55729_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 19533_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 19533_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 187029_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 187029_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 125061_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 125061_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 84615_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 84615_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:46:31.73 +35:40:06.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56963_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 56963_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 60287_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 60287_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 157084_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 157084_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:47:05.39 +37:55:41.4 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 77385_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 77385_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 61070_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 61070_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:12:01.37 +34:54:06.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 38232_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 38232_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:38:41.55 +34:03:37.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 115059_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 115059_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 73129_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 73129_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:26:02.06 +35:03:04.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 110172_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 110172_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 196821_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 196821_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 52707_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 52707_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 29558_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 29558_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 127787_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 127787_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 188769_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 188769_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:51:48.90 +39:00:35.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 41459_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 41459_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 109021_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 109021_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 65878_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 65878_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:11:05.69 +35:04:51.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 1.157 2058772060579251072 302.77356810311 +35.08116138250 12.6709 11.1930 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.157#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 222033_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 222033_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 73270_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 73270_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:58:42.07 +35:21:23.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 3.276 2059392223811688960 299.67550718353 +35.35730955648 12.2107 10.6503 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.276#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 288606_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 288606_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 54865_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 54865_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 202376_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 202376_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 55879_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 55879_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 311071_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 311071_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:21:07.08 +35:18:54.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 4.772 2050003287848735104 290.27809039900 +35.31577022618 12.1639 10.5883 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.772#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 81005_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 81005_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 158870_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 158870_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 33510_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 33510_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 21215_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 21215_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 73318_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 73318_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 51759_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 51759_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 173362_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 173362_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 09355_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 09355_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 12707_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 12707_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 42197_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 42197_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 94725_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 94725_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 102690_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 102690_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 260449_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 260449_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 49821_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 49821_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 132952_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 132952_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 246854_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 246854_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 286316_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 286316_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 101309_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 101309_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 56879_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 56879_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:47:46.36 +34:42:06.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 210606_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 210606_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:44:09.46 +39:47:24.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71166_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 71166_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:53:59.00 +35:17:08.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 5.508 2035556357923518336 298.49743428762 +35.28660124221 12.2018 10.6534 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.508#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 185106_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 185106_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:16:38.43 +38:49:08.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 4.401 2061340489697074304 304.16162820670 +38.81923948156 13.2062 11.9028 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.401#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 226819_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 226819_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 142778_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 142778_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 19964_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 19964_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 59158_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 59158_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 12451_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 12451_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:58:12.20 +33:12:30.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 87178_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 87178_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 208211_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 208211_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 09994_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 09994_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 199627_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 199627_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 125538_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 125538_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 34119_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 34119_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:13:01.43 +33:24:49.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 135872_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 135872_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 128935_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 128935_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 160836_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 160836_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 63751_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 63751_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:09:34.67 +34:58:42.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 166578_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 166578_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 50541_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 50541_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 171075_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 171075_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 33745_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 33745_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 91449_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 91449_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 135937_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 135937_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 169010_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 169010_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 92326_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 92326_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 15342_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 15342_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 95549_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 95549_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 308457_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 308457_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:55:14.49 +37:13:08.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 0.907 2071902428437005440 298.81022184004 +37.21919262217 12.2440 10.7666 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.907#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 113369_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 113369_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:24:57.93 +36:12:54.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 55255_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 55255_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 154816_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 154816_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:53:32.85 +37:51:45.0 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 32043_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 32043_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 104664_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 104664_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 89143_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 89143_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 127418_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 127418_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 55516_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 55516_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 115989_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 115989_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 131382_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 131382_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:12:39.63 +37:06:53.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.50, MAG_FAINT_SEARCH_LIMIT=13.48)GAIADR2_OUTPUT=# 2.406 2060735655227278592 303.16596286114 +37.11482155676 12.0634 10.8187 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.406#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 44527_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 44527_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:24:04.20 +34:03:31.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 31271_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 31271_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:49:10.61 +33:53:40.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 2.867 2035366894003682688 297.29478127086 +33.89516641306 12.5647 11.1727 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.867#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 307609_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 307609_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:26:54.22 +37:58:06.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 3.552 2052563569391302784 291.72622957666 +37.96951092757 12.0802 10.5289 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.552#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 19013_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 19013_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 99753_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 99753_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:00:13.30 +36:08:44.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 15833_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 15833_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 274160_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 274160_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 77969_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 77969_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 119025_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 119025_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 306740_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 306740_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:52:55.55 +36:19:24.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 4.096 2071709979542620672 298.23186598795 +36.32456161469 12.5940 11.2464 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.096#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 197724_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 197724_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 118674_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 118674_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 120333_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 120333_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 67200_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 67200_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 24649_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 24649_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 46722_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 46722_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:41:15.65 +34:21:55.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.33, MAG_FAINT_SEARCH_LIMIT=13.31)
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Considering the candidate 48990_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 48990_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:36:15.11 +34:23:48.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 1.337 2048014821077301760 294.06281185577 +34.39715684960 11.3581 9.8390 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.337#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 34419_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 34419_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 81331_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 81331_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 306145_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 306145_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:04:20.97 +37:01:14.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 3.924 2060062857196999936 301.08790892662 +37.02158642491 12.2962 10.8007 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.924#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 27542_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 27542_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
Rejecting candidate due to large distance (17.8") between the two second-epoch detections
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Considering the candidate 305949_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 305949_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:16:11.14 +36:42:43.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.70, MAG_FAINT_SEARCH_LIMIT=13.68)GAIADR2_OUTPUT=# 1.173 2060466407996436864 304.04666593333 +36.71231290085 12.3606 11.7574 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.173#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 16389_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 16389_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 194813_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 194813_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:45:19.69 +39:12:25.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.81, MAG_FAINT_SEARCH_LIMIT=12.79)GAIADR2_OUTPUT=# 2.524 2073276302574410112 296.33114200611 +39.20726966340 12.0008 11.2572 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.524#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 92989_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 92989_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 15426_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 15426_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 53521_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 53521_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 31823_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 31823_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 45122_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 45122_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 44167_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 44167_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 179142_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 179142_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 12222_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 12222_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 52336_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 52336_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 23691_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 23691_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:19:15.21 +33:14:45.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 92336_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 92336_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:03:32.86 +35:56:55.3 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 212675_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 212675_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 36500_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 36500_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 17213_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 17213_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 131470_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 131470_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 304603_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 304603_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 121652_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 121652_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 193423_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 193423_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 116539_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 116539_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:02:26.04 +36:42:08.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.33, MAG_FAINT_SEARCH_LIMIT=13.31)GAIADR2_OUTPUT=# 5.646 2059938092657765632 300.61035103231 +36.70281303943 13.2832 12.8352 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.646#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 76628_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 76628_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 218572_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 218572_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 27474_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 27474_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 304201_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 304201_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:01:22.88 +39:47:46.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 5.388 2074202542360409600 300.34444846125 +39.79752763490 12.2905 10.7507 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.388#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 92047_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 92047_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 276789_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 276789_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:20:08.74 +41:40:57.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234153_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 234153_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 22446_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 22446_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 161477_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 161477_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 182293_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 182293_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 68574_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 68574_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 60982_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 60982_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:51:43.30 +34:55:54.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 2.853 2035567593559014528 297.93064645726 +34.93265869416 12.4040 10.9227 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.853#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 34540_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 34540_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 255055_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 255055_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 27414_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 27414_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 192393_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 192393_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 185903_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 185903_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 110023_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 110023_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 233771_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 233771_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:47:34.82 +40:44:08.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 127582_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 127582_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 62681_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 62681_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:07:59.46 +34:58:57.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)
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Considering the candidate 209353_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 209353_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 303188_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 303188_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 61872_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 61872_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:27:43.41 +34:43:08.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)
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Considering the candidate 161533_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 161533_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 229624_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 229624_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 113678_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 113678_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 222507_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 222507_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 44412_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 44412_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 44867_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 44867_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 66131_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 66131_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 114081_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 114081_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:25:50.74 +36:21:26.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 4.788 2050166462246160128 291.46133405212 +36.35871725742 13.9933 11.5836 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.788#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 219427_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 219427_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 302939_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 302939_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 302754_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 302754_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:45:02.17 +35:46:11.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)
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Considering the candidate 118843_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 118843_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 225192_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 225192_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 165109_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 165109_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 302579_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 302579_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 182674_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 182674_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:43:10.70 +38:40:17.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 39727_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 39727_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 131788_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 131788_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:35:48.41 +36:56:42.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 76844_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 76844_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:36:07.46 +35:12:48.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 79348_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 79348_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:38:01.52 +35:15:33.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 144424_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 144424_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:44:16.64 +37:21:16.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 36150_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 36150_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
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Considering the candidate 173848_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 173848_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:47:27.65 +38:24:30.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 182268_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 182268_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:49:27.34 +38:42:38.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 110717_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 110717_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:30:47.03 +36:13:45.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 101247_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 101247_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:45:39.90 +36:05:27.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 72044_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 72044_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:37:40.86 +35:01:23.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 111692_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 111692_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:52:16.21 +36:25:57.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 117634_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 117634_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:26:09.52 +36:19:05.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 68745_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 68745_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:45:51.37 +35:00:50.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 35843_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 35843_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:30:17.39 +33:43:43.5 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 129101_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 129101_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:54:48.00 +36:59:44.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 232930_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 232930_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:50:37.13 +40:35:55.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 44456_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 44456_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:43:51.43 +34:09:49.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 106363_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 106363_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:56:43.95 +36:15:03.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 38771_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 38771_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:39:44.93 +33:58:47.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 279687_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 279687_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:43:45.09 +41:46:20.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 36538_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 36538_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:34:56.20 +33:47:46.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 30603_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 30603_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:54:09.66 +33:46:53.8 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131938_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 131938_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:01:15.24 +37:05:58.6 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 226806_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 226806_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:57:13.43 +40:22:05.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70283_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 70283_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:56:17.97 +35:05:03.4 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19017_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 19017_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 302384_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 302384_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 19:52:42.57 +35:52:32.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 122243_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
Preparing report for the candidate 122243_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 96526_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 96526_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:06:21.09 +35:58:10.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 127508_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 127508_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:09:25.41 +36:50:24.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 229840_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 229840_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:16:55.04 +40:21:52.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125268_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187
The candidate 125268_fd_Cyg-05-Q1b1x1_2026-04-09_02-24-44_20.00sec_-5.00C_LIGHTs_0187 did not pass the final checks
**** FOUND 20:14:32.08 +36:48:24.6 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 21s
make_report_in_HTML.sh TOTAL: 351s
Prepared the HTML report for the field Cyg-05-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
19:47:46.36 +34:42:07.2
20:03:33.00 +35:56:57.7
19:35:21.60 +36:04:03.3
19:24:57.98 +36:12:55.7
20:06:01.25 +37:14:30.0
19:53:32.84 +37:51:45.6
19:47:05.35 +37:55:42.3
19:55:13.31 +39:33:00.9
19:51:33.52 +40:39:37.4
19:48:26.68 +42:47:33.0
20:08:49.80 +35:30:51.7
19:29:08.06 +40:44:41.8
19:05:45.47 +37:04:10.9
19:42:56.07 +32:55:33.7
20:13:19.41 +32:57:25.2
19:41:46.32 +33:01:18.2
19:41:55.32 +33:04:20.9
19:45:16.60 +33:06:50.6
19:50:20.66 +36:11:06.2
20:04:22.43 +36:08:42.3
19:59:53.44 +36:16:36.1
19:25:28.56 +36:01:04.3
19:40:43.02 +36:13:35.1
19:08:09.60 +35:40:03.4
20:02:35.01 +36:25:58.2
19:02:40.40 +35:38:22.2
20:12:41.27 +36:27:05.4
19:36:41.76 +36:22:30.5
19:48:00.72 +36:25:50.5
20:02:37.25 +36:34:49.4
20:02:39.75 +36:36:38.5
19:06:04.52 +35:56:17.0
19:44:09.66 +36:35:55.6
19:47:56.92 +36:39:51.6
19:40:33.41 +36:40:22.5
19:49:04.87 +36:43:59.5
20:00:29.30 +36:46:08.9
19:35:24.79 +36:39:08.2
19:50:09.68 +36:46:40.4
19:35:53.60 +36:36:54.9
19:41:07.44 +36:43:09.4
20:01:50.42 +36:49:15.4
19:40:58.96 +36:43:28.6
19:59:16.30 +36:50:00.8
19:49:06.09 +36:50:52.9
19:52:24.44 +33:15:03.8
20:10:00.43 +36:51:09.2
19:48:18.95 +36:57:05.2
19:52:37.87 +36:57:45.7
19:56:42.03 +37:00:26.7
19:46:47.18 +36:57:31.1
19:15:50.47 +36:32:20.7
19:30:39.54 +36:50:05.9
19:28:16.85 +33:01:14.5
19:07:49.10 +36:23:06.5
20:09:15.19 +37:01:43.8
19:58:33.06 +37:03:11.2
19:41:53.20 +37:00:31.6
19:56:36.08 +37:05:23.9
20:04:24.21 +37:07:17.9
19:34:27.81 +37:00:51.6
19:44:32.46 +37:10:01.4
20:11:14.89 +37:14:20.7
19:51:20.58 +37:18:28.9
19:50:53.66 +37:13:54.2
20:12:24.05 +37:19:53.2
20:07:32.70 +37:21:45.7
20:01:44.11 +37:27:42.1
19:03:58.01 +36:45:27.7
19:38:56.08 +37:26:01.3
19:31:06.87 +33:07:12.0
20:03:04.91 +37:32:26.1
19:42:20.33 +37:28:13.6
19:50:52.85 +37:40:46.6
19:52:36.27 +37:50:02.8
19:12:08.80 +37:18:22.2
19:33:40.81 +33:11:57.9
19:44:24.92 +33:18:28.5
19:59:10.82 +33:23:37.8
19:50:43.13 +33:21:10.6
19:29:05.69 +37:47:19.7
19:36:38.89 +37:55:58.0
19:10:05.83 +37:30:27.8
20:02:56.80 +38:07:46.7
19:42:06.64 +38:03:33.7
19:25:00.07 +37:54:05.5
19:50:07.56 +33:20:57.0
19:25:05.42 +33:06:29.5
19:29:44.02 +33:10:32.7
19:54:33.29 +38:14:44.8
19:42:00.95 +38:11:33.7
20:03:10.21 +38:17:20.8
19:45:16.98 +38:16:31.3
20:11:23.75 +38:17:04.3
20:02:21.44 +38:21:04.3
19:53:54.33 +38:24:49.8
20:09:46.62 +38:24:41.3
20:13:00.23 +33:23:50.4
19:43:54.51 +38:26:44.6
20:15:39.34 +38:25:40.6
19:52:36.92 +38:35:11.7
20:16:13.52 +38:36:52.0
19:45:06.97 +38:47:03.3
20:12:45.35 +33:25:41.7
19:42:08.24 +33:23:39.3
20:15:51.65 +38:51:09.3
19:52:22.24 +38:58:40.0
20:10:33.86 +33:27:23.6
20:13:01.79 +33:26:44.4
19:44:23.24 +33:24:50.6
20:11:08.02 +39:06:50.7
19:52:33.75 +33:29:22.1
19:55:23.65 +39:12:55.7
19:37:49.36 +33:23:19.3
19:48:27.84 +39:16:33.9
20:01:57.94 +39:21:10.0
19:34:53.84 +39:18:12.4
19:51:17.64 +33:30:38.4
20:12:10.83 +39:26:10.7
19:45:17.12 +39:30:34.5
20:04:07.76 +39:37:20.2
19:50:21.35 +33:31:37.0
19:52:51.63 +39:43:22.3
19:56:01.49 +39:43:10.7
19:27:31.48 +39:33:57.9
19:27:10.56 +33:18:05.2
19:44:19.77 +39:52:58.3
19:49:50.41 +33:33:37.1
19:41:31.00 +40:00:51.3
19:43:55.09 +40:06:36.6
20:06:27.19 +40:08:48.0
19:37:55.01 +40:11:46.3
20:14:04.75 +40:12:40.2
19:45:25.74 +40:15:37.2
20:06:10.97 +33:36:22.9
19:48:35.46 +40:26:50.3
19:16:12.76 +33:08:41.0
20:02:53.78 +40:30:18.2
20:03:29.86 +40:34:26.9
20:00:43.13 +40:38:04.4
19:54:07.89 +40:40:38.8
20:01:47.38 +40:46:02.4
19:32:32.41 +40:44:53.8
19:31:55.38 +33:29:44.6
20:03:03.23 +41:08:19.0
20:04:22.09 +41:02:12.9
19:01:42.64 +42:17:10.4
19:31:51.32 +42:45:04.1
20:03:53.45 +33:46:55.1
19:49:43.36 +42:12:13.6
19:31:10.45 +33:34:59.6
19:48:00.70 +33:46:05.9
19:43:08.78 +41:34:10.0
20:13:11.69 +41:27:21.1
19:52:53.57 +41:30:04.1
19:55:19.52 +41:32:17.4
19:34:32.40 +33:41:24.7
19:39:17.42 +33:45:22.6
19:28:16.60 +33:36:44.6
19:47:28.83 +39:09:58.6
19:19:30.98 +33:27:37.3
19:57:40.90 +36:01:14.2
19:45:40.65 +42:35:22.7
19:30:48.02 +38:57:28.2
20:10:35.81 +35:41:49.1
19:46:40.53 +33:53:54.5
20:10:08.56 +33:55:27.1
20:05:30.72 +37:39:35.4
19:50:40.36 +39:25:24.9
20:14:32.40 +39:33:17.3
20:12:50.30 +35:19:36.0
19:47:48.48 +36:19:12.9
19:36:58.41 +33:22:26.4
19:44:11.71 +40:27:11.1
19:43:31.05 +38:33:51.2
19:44:03.16 +36:09:46.1
20:02:29.79 +37:05:55.9
19:40:24.09 +41:51:45.0
19:10:17.36 +34:22:33.3
19:56:32.48 +38:50:19.3
20:05:43.79 +40:04:30.5
19:44:26.98 +35:50:28.5
20:15:50.05 +39:06:36.4
19:55:55.49 +36:03:07.9
19:34:45.43 +35:14:13.2
19:37:09.26 +37:54:12.6
19:51:00.93 +36:24:04.4
20:02:37.35 +35:20:13.8
19:54:12.51 +37:52:30.1
19:42:14.32 +33:59:33.8
20:06:06.18 +39:09:31.3
19:48:57.84 +33:11:30.0
20:12:06.60 +36:24:46.7
20:03:53.28 +39:52:36.1
20:03:35.80 +37:35:08.9
19:52:09.66 +38:58:20.5
20:17:30.70 +38:28:42.8
20:12:32.34 +37:01:28.9
20:14:40.17 +36:35:15.5
20:09:08.99 +33:27:24.9
19:59:47.81 +33:23:42.6
20:14:09.86 +37:43:22.2
19:43:59.10 +34:01:50.6
20:13:30.20 +33:53:36.3
20:11:58.84 +33:47:59.0
20:12:56.06 +32:57:06.9
20:13:21.17 +33:02:49.7
20:13:13.24 +33:17:31.6
20:13:25.78 +32:55:18.9
20:12:41.82 +33:00:51.7
20:11:49.26 +32:48:37.8
20:16:18.55 +37:55:39.4
20:14:21.18 +36:09:56.5
20:19:30.95 +41:58:23.6
19:05:01.07 +35:01:55.7
20:03:58.64 +38:25:33.2
20:12:36.83 +34:24:11.7
19:38:19.96 +40:52:42.8
20:13:24.65 +33:11:31.4
19:42:56.08 +37:41:58.7
19:08:14.40 +42:06:33.5
20:00:09.09 +39:24:58.8
19:47:29.81 +34:50:04.7
19:19:10.76 +35:18:03.3
20:11:23.97 +37:54:20.3
20:08:49.21 +39:04:25.0
20:01:23.13 +40:06:31.5
19:42:38.13 +33:55:56.9
19:24:36.76 +33:42:50.9
20:01:09.67 +34:01:18.2
19:49:34.33 +34:00:11.5
20:13:14.72 +34:01:23.3
20:03:01.62 +34:05:05.8
19:54:23.41 +34:04:49.3
19:40:41.68 +34:03:15.2
19:37:02.54 +34:03:10.0
19:55:53.73 +34:10:49.3
19:56:28.16 +34:10:44.7
19:57:58.89 +34:12:52.5
20:05:39.41 +34:15:17.4
19:47:49.78 +34:14:41.7
20:02:33.70 +34:22:12.1
19:05:48.27 +33:36:30.3
19:34:44.72 +34:13:09.0
19:44:27.15 +34:19:42.0
19:48:45.74 +34:21:55.1
19:46:36.21 +34:21:31.3
19:46:55.55 +34:23:34.4
20:11:54.95 +34:24:07.7
19:50:33.34 +34:32:01.5
20:08:30.09 +34:31:54.6
19:19:53.30 +34:10:46.3
19:42:03.54 +34:32:28.8
19:40:55.93 +34:31:40.8
19:37:51.16 +34:31:20.9
19:47:41.68 +34:35:58.7
20:12:06.16 +34:38:32.5
19:31:29.11 +34:31:59.9
20:13:03.57 +34:41:39.5
20:05:00.74 +34:45:07.5
19:58:40.84 +34:45:40.2
20:12:02.14 +34:43:30.1
19:53:40.69 +34:47:35.8
20:11:21.50 +34:45:58.9
19:42:56.73 +34:44:58.0
19:34:28.39 +34:43:07.9
19:51:58.84 +34:54:01.1
20:05:37.09 +34:53:31.4
19:46:42.35 +34:50:39.0
19:09:08.22 +34:26:58.1
19:27:35.37 +34:49:30.0
20:12:06.40 +35:03:11.6
19:46:18.51 +35:03:46.6
20:03:18.43 +35:07:54.8
20:14:28.93 +35:06:32.2
19:50:45.11 +35:11:04.8
19:23:19.20 +35:01:44.8
19:42:39.47 +35:17:05.2
19:49:50.58 +35:20:40.7
19:34:46.33 +35:13:28.8
19:50:43.26 +35:26:56.2
19:24:26.79 +35:11:09.3
20:14:37.70 +35:26:28.2
20:01:57.03 +35:33:03.8
19:58:23.20 +35:34:15.1
19:59:29.20 +35:36:14.1
19:45:50.57 +35:34:08.3
20:08:11.42 +35:36:05.2
19:32:23.66 +35:30:26.1
20:13:13.78 +35:42:30.6
20:14:53.18 +35:43:57.8
20:02:24.23 +35:48:38.8
20:08:06.48 +35:47:53.8
19:27:01.76 +35:35:31.4
19:40:32.32 +35:50:48.9
19:54:49.40 +35:55:51.9
20:00:23.29 +35:57:25.7
20:12:08.19 +35:56:12.0
20:01:50.40 +36:00:49.9
19:30:59.97 +35:48:34.2
20:00:13.07 +36:03:28.3
19:01:43.19 +35:13:38.2
19:40:09.53 +36:00:27.7
########### Completed Cyg-05-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
20:08:49.80 +35:30:51.7
19:29:08.06 +40:44:41.8
19:05:45.47 +37:04:10.9
20:06:01.25 +37:14:30.0
19:35:21.60 +36:04:03.3
20:03:33.00 +35:56:57.7
19:51:33.52 +40:39:37.4
19:24:57.98 +36:12:55.7
19:48:26.68 +42:47:33.0
19:47:46.36 +34:42:07.2
19:47:05.35 +37:55:42.3
19:55:13.31 +39:33:00.9
19:53:32.84 +37:51:45.6
20:05:30.72 +37:39:35.4
19:50:40.36 +39:25:24.9
20:14:32.40 +39:33:17.3
20:12:50.30 +35:19:36.0
19:47:48.48 +36:19:12.9
19:36:58.41 +33:22:26.4
19:44:11.71 +40:27:11.1
19:43:31.05 +38:33:51.2
19:44:03.16 +36:09:46.1
20:02:29.79 +37:05:55.9
19:40:24.09 +41:51:45.0
19:10:17.36 +34:22:33.3
19:56:32.48 +38:50:19.3
20:05:43.79 +40:04:30.5
19:44:26.98 +35:50:28.5
20:15:50.05 +39:06:36.4
19:55:55.49 +36:03:07.9
19:34:45.43 +35:14:13.2
19:37:09.26 +37:54:12.6
19:51:00.93 +36:24:04.4
20:02:37.35 +35:20:13.8
19:54:12.51 +37:52:30.1
19:42:14.32 +33:59:33.8
20:06:06.18 +39:09:31.3
19:48:57.84 +33:11:30.0
20:12:06.60 +36:24:46.7
20:03:53.28 +39:52:36.1
20:03:35.80 +37:35:08.9
19:52:09.66 +38:58:20.5
20:17:30.70 +38:28:42.8
20:12:32.34 +37:01:28.9
20:14:40.17 +36:35:15.5
20:09:08.99 +33:27:24.9
19:59:47.81 +33:23:42.6
20:14:09.86 +37:43:22.2
19:43:59.10 +34:01:50.6
20:13:30.20 +33:53:36.3
20:11:58.84 +33:47:59.0
20:12:56.06 +32:57:06.9
20:13:21.17 +33:02:49.7
20:13:13.24 +33:17:31.6
20:13:25.78 +32:55:18.9
20:12:41.82 +33:00:51.7
20:11:49.26 +32:48:37.8
20:16:18.55 +37:55:39.4
20:14:21.18 +36:09:56.5
20:19:30.95 +41:58:23.6
19:05:01.07 +35:01:55.7
20:03:58.64 +38:25:33.2
20:12:36.83 +34:24:11.7
19:38:19.96 +40:52:42.8
20:13:24.65 +33:11:31.4
19:42:56.08 +37:41:58.7
19:08:14.40 +42:06:33.5
20:00:09.09 +39:24:58.8
19:47:29.81 +34:50:04.7
19:19:10.76 +35:18:03.3
20:11:23.97 +37:54:20.3
20:08:49.21 +39:04:25.0
20:01:23.13 +40:06:31.5
19:43:54.51 +38:26:44.6
19:23:19.20 +35:01:44.8
19:55:53.73 +34:10:49.3
19:42:56.07 +32:55:33.7
19:12:08.80 +37:18:22.2
19:46:47.18 +36:57:31.1
19:45:16.98 +38:16:31.3
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19:47:49.78 +34:14:41.7
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19:51:20.58 +37:18:28.9
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20:03:10.21 +38:17:20.8
19:19:53.30 +34:10:46.3
20:09:46.62 +38:24:41.3
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19:40:32.32 +35:50:48.9
19:50:53.66 +37:13:54.2
20:02:21.44 +38:21:04.3
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20:00:13.07 +36:03:28.3
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20:10:08.56 +33:55:27.1
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20:14:37.70 +35:26:28.2
19:35:24.79 +36:39:08.2
20:01:57.94 +39:21:10.0
19:49:04.87 +36:43:59.5
20:01:50.42 +36:49:15.4
20:03:18.43 +35:07:54.8
19:31:55.38 +33:29:44.6
20:01:09.67 +34:01:18.2
19:45:50.57 +35:34:08.3
19:50:07.56 +33:20:57.0
20:12:08.19 +35:56:12.0
19:44:24.92 +33:18:28.5
20:12:06.16 +34:38:32.5
19:46:40.53 +33:53:54.5
19:46:36.21 +34:21:31.3
20:02:33.70 +34:22:12.1
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19:52:24.44 +33:15:03.8
19:37:51.16 +34:31:20.9
19:44:19.77 +39:52:58.3
19:54:23.41 +34:04:49.3
20:13:00.23 +33:23:50.4
20:04:24.21 +37:07:17.9
20:10:35.81 +35:41:49.1
19:49:06.09 +36:50:52.9
19:55:23.65 +39:12:55.7
19:50:43.26 +35:26:56.2
19:43:55.09 +40:06:36.6
19:31:10.45 +33:34:59.6
19:54:49.40 +35:55:51.9
20:01:47.38 +40:46:02.4
20:06:10.97 +33:36:22.9
20:02:56.80 +38:07:46.7
19:45:06.97 +38:47:03.3
19:50:45.11 +35:11:04.8
19:49:34.33 +34:00:11.5
19:01:42.64 +42:17:10.4
20:03:53.45 +33:46:55.1
20:11:08.02 +39:06:50.7
20:15:51.65 +38:51:09.3
20:12:41.27 +36:27:05.4
20:09:15.19 +37:01:43.8
19:27:31.48 +39:33:57.9
19:30:48.02 +38:57:28.2
19:42:06.64 +38:03:33.7
20:03:29.86 +40:34:26.9
20:02:39.75 +36:36:38.5
20:14:04.75 +40:12:40.2
19:05:48.27 +33:36:30.3
19:44:27.15 +34:19:42.0
19:46:18.51 +35:03:46.6
20:06:27.19 +40:08:48.0
19:45:40.65 +42:35:22.7
20:00:29.30 +36:46:08.9
19:54:33.29 +38:14:44.8
19:57:40.90 +36:01:14.2
19:57:58.89 +34:12:52.5
20:03:01.62 +34:05:05.8
20:13:01.79 +33:26:44.4
20:10:00.43 +36:51:09.2
###################################################################################
20:08:49.80 +35:30:51.7 -- not an asteroid (will add it to exclusion list)
19:29:08.06 +40:44:41.8 -- not an asteroid (will add it to exclusion list)
19:05:45.47 +37:04:10.9 -- not an asteroid (will add it to exclusion list)
20:06:01.25 +37:14:30.0 -- not an asteroid (will add it to exclusion list)
19:35:21.60 +36:04:03.3 -- not an asteroid (will add it to exclusion list)
20:03:33.00 +35:56:57.7 -- not an asteroid (will add it to exclusion list)
19:51:33.52 +40:39:37.4 -- not an asteroid (will add it to exclusion list)
19:24:57.98 +36:12:55.7 -- not an asteroid (will add it to exclusion list)
19:48:26.68 +42:47:33.0 -- not an asteroid (will add it to exclusion list)
19:47:46.36 +34:42:07.2 -- not an asteroid (will add it to exclusion list)
19:47:05.35 +37:55:42.3 -- not an asteroid (will add it to exclusion list)
19:55:13.31 +39:33:00.9 -- not an asteroid (will add it to exclusion list)
19:53:32.84 +37:51:45.6 -- not an asteroid (will add it to exclusion list)
20:05:30.72 +37:39:35.4 -- not an asteroid (will add it to exclusion list)
19:50:40.36 +39:25:24.9 -- not an asteroid (will add it to exclusion list)
20:14:32.40 +39:33:17.3 -- not an asteroid (will add it to exclusion list)
20:12:50.30 +35:19:36.0 -- not an asteroid (will add it to exclusion list)
19:47:48.48 +36:19:12.9 -- not an asteroid (will add it to exclusion list)
19:36:58.41 +33:22:26.4 -- not an asteroid (will add it to exclusion list)
19:44:11.71 +40:27:11.1 -- not an asteroid (will add it to exclusion list)
19:43:31.05 +38:33:51.2 -- not an asteroid (will add it to exclusion list)
19:44:03.16 +36:09:46.1 -- not an asteroid (will add it to exclusion list)
20:02:29.79 +37:05:55.9 -- not an asteroid (will add it to exclusion list)
19:40:24.09 +41:51:45.0 -- not an asteroid (will add it to exclusion list)
19:10:17.36 +34:22:33.3 -- not an asteroid (will add it to exclusion list)
19:56:32.48 +38:50:19.3 -- not an asteroid (will add it to exclusion list)
20:05:43.79 +40:04:30.5 -- not an asteroid (will add it to exclusion list)
19:44:26.98 +35:50:28.5 -- not an asteroid (will add it to exclusion list)
20:15:50.05 +39:06:36.4 -- not an asteroid (will add it to exclusion list)
19:55:55.49 +36:03:07.9 -- not an asteroid (will add it to exclusion list)
19:34:45.43 +35:14:13.2 -- not an asteroid (will add it to exclusion list)
19:37:09.26 +37:54:12.6 -- not an asteroid (will add it to exclusion list)
19:51:00.93 +36:24:04.4 -- not an asteroid (will add it to exclusion list)
20:02:37.35 +35:20:13.8 -- not an asteroid (will add it to exclusion list)
19:54:12.51 +37:52:30.1 -- not an asteroid (will add it to exclusion list)
19:42:14.32 +33:59:33.8 -- not an asteroid (will add it to exclusion list)
20:06:06.18 +39:09:31.3 -- not an asteroid (will add it to exclusion list)
19:48:57.84 +33:11:30.0 -- not an asteroid (will add it to exclusion list)
20:12:06.60 +36:24:46.7 -- not an asteroid (will add it to exclusion list)
20:03:53.28 +39:52:36.1 -- not an asteroid (will add it to exclusion list)
20:03:35.80 +37:35:08.9 -- not an asteroid (will add it to exclusion list)
19:52:09.66 +38:58:20.5 -- not an asteroid (will add it to exclusion list)
20:17:30.70 +38:28:42.8 -- not an asteroid (will add it to exclusion list)
20:12:32.34 +37:01:28.9 -- not an asteroid (will add it to exclusion list)
20:14:40.17 +36:35:15.5 -- not an asteroid (will add it to exclusion list)
20:09:08.99 +33:27:24.9 -- not an asteroid (will add it to exclusion list)
19:59:47.81 +33:23:42.6 -- not an asteroid (will add it to exclusion list)
20:14:09.86 +37:43:22.2 -- not an asteroid (will add it to exclusion list)
19:43:59.10 +34:01:50.6 -- not an asteroid (will add it to exclusion list)
20:13:30.20 +33:53:36.3 -- not an asteroid (will add it to exclusion list)
20:11:58.84 +33:47:59.0 -- not an asteroid (will add it to exclusion list)
20:12:56.06 +32:57:06.9 -- not an asteroid (will add it to exclusion list)
20:13:21.17 +33:02:49.7 -- not an asteroid (will add it to exclusion list)
20:13:13.24 +33:17:31.6 -- not an asteroid (will add it to exclusion list)
20:13:25.78 +32:55:18.9 -- not an asteroid (will add it to exclusion list)
20:12:41.82 +33:00:51.7 -- not an asteroid (will add it to exclusion list)
20:11:49.26 +32:48:37.8 -- not an asteroid (will add it to exclusion list)
20:16:18.55 +37:55:39.4 -- not an asteroid (will add it to exclusion list)
20:14:21.18 +36:09:56.5 -- not an asteroid (will add it to exclusion list)
20:19:30.95 +41:58:23.6 -- not an asteroid (will add it to exclusion list)
19:05:01.07 +35:01:55.7 -- not an asteroid (will add it to exclusion list)
20:03:58.64 +38:25:33.2 -- not an asteroid (will add it to exclusion list)
20:12:36.83 +34:24:11.7 -- not an asteroid (will add it to exclusion list)
19:38:19.96 +40:52:42.8 -- not an asteroid (will add it to exclusion list)
20:13:24.65 +33:11:31.4 -- not an asteroid (will add it to exclusion list)
19:42:56.08 +37:41:58.7 -- not an asteroid (will add it to exclusion list)
19:08:14.40 +42:06:33.5 -- not an asteroid (will add it to exclusion list)
20:00:09.09 +39:24:58.8 -- not an asteroid (will add it to exclusion list)
19:47:29.81 +34:50:04.7 -- not an asteroid (will add it to exclusion list)
19:19:10.76 +35:18:03.3 -- not an asteroid (will add it to exclusion list)
20:11:23.97 +37:54:20.3 -- not an asteroid (will add it to exclusion list)
20:08:49.21 +39:04:25.0 -- not an asteroid (will add it to exclusion list)
20:01:23.13 +40:06:31.5 -- not an asteroid (will add it to exclusion list)
19:43:54.51 +38:26:44.6 -- not an asteroid (will add it to exclusion list)
19:23:19.20 +35:01:44.8 -- not an asteroid (will add it to exclusion list)
19:55:53.73 +34:10:49.3 -- not an asteroid (will add it to exclusion list)
19:42:56.07 +32:55:33.7 -- not an asteroid (will add it to exclusion list)
19:12:08.80 +37:18:22.2 -- not an asteroid (will add it to exclusion list)
19:46:47.18 +36:57:31.1 -- not an asteroid (will add it to exclusion list)
19:45:16.98 +38:16:31.3 -- not an asteroid (will add it to exclusion list)
20:11:23.75 +38:17:04.3 -- not an asteroid (will add it to exclusion list)
19:30:39.54 +36:50:05.9 -- not an asteroid (will add it to exclusion list)
19:09:08.22 +34:26:58.1 -- not an asteroid (will add it to exclusion list)
19:41:31.00 +40:00:51.3 -- not an asteroid (will add it to exclusion list)
19:48:27.84 +39:16:33.9 -- not an asteroid (will add it to exclusion list)
20:12:45.35 +33:25:41.7 -- not an asteroid (will add it to exclusion list)
20:04:22.09 +41:02:12.9 -- not an asteroid (will add it to exclusion list)
19:42:00.95 +38:11:33.7 -- not an asteroid (will add it to exclusion list)
19:25:00.07 +37:54:05.5 -- not an asteroid (will add it to exclusion list)
19:25:05.42 +33:06:29.5 -- not an asteroid (will add it to exclusion list)
19:34:44.72 +34:13:09.0 -- not an asteroid (will add it to exclusion list)
19:29:44.02 +33:10:32.7 -- not an asteroid (will add it to exclusion list)
19:52:36.27 +37:50:02.8 -- not an asteroid (will add it to exclusion list)
19:42:56.73 +34:44:58.0 -- not an asteroid (will add it to exclusion list)
19:52:33.75 +33:29:22.1 -- not an asteroid (will add it to exclusion list)
19:46:55.55 +34:23:34.4 -- not an asteroid (will add it to exclusion list)
19:50:20.66 +36:11:06.2 -- not an asteroid (will add it to exclusion list)
20:00:43.13 +40:38:04.4 -- not an asteroid (will add it to exclusion list)
19:35:53.60 +36:36:54.9 -- not an asteroid (will add it to exclusion list)
20:12:10.83 +39:26:10.7 -- not an asteroid (will add it to exclusion list)
19:27:35.37 +34:49:30.0 -- not an asteroid (will add it to exclusion list)
19:31:06.87 +33:07:12.0 -- not an asteroid (will add it to exclusion list)
20:13:11.69 +41:27:21.1 -- not an asteroid (will add it to exclusion list)
19:16:12.76 +33:08:41.0 -- not an asteroid (will add it to exclusion list)
19:55:19.52 +41:32:17.4 -- not an asteroid (will add it to exclusion list)
19:48:00.72 +36:25:50.5 -- not an asteroid (will add it to exclusion list)
20:03:04.91 +37:32:26.1 -- not an asteroid (will add it to exclusion list)
19:40:43.02 +36:13:35.1 -- not an asteroid (will add it to exclusion list)
19:47:28.83 +39:09:58.6 -- not an asteroid (will add it to exclusion list)
19:03:58.01 +36:45:27.7 -- not an asteroid (will add it to exclusion list)
19:48:45.74 +34:21:55.1 -- not an asteroid (will add it to exclusion list)
20:02:35.01 +36:25:58.2 -- not an asteroid (will add it to exclusion list)
19:52:51.63 +39:43:22.3 -- not an asteroid (will add it to exclusion list)
20:14:28.93 +35:06:32.2 -- not an asteroid (will add it to exclusion list)
19:53:40.69 +34:47:35.8 -- not an asteroid (will add it to exclusion list)
20:12:24.05 +37:19:53.2 -- not an asteroid (will add it to exclusion list)
20:12:06.40 +35:03:11.6 -- not an asteroid (will add it to exclusion list)
19:48:00.70 +33:46:05.9 -- not an asteroid (will add it to exclusion list)
19:15:50.47 +36:32:20.7 -- not an asteroid (will add it to exclusion list)
19:30:59.97 +35:48:34.2 -- not an asteroid (will add it to exclusion list)
19:49:50.41 +33:33:37.1 -- not an asteroid (will add it to exclusion list)
19:56:42.03 +37:00:26.7 -- not an asteroid (will add it to exclusion list)
20:13:13.78 +35:42:30.6 -- not an asteroid (will add it to exclusion list)
19:41:46.32 +33:01:18.2 -- not an asteroid (will add it to exclusion list)
19:44:23.24 +33:24:50.6 -- not an asteroid (will add it to exclusion list)
19:50:21.35 +33:31:37.0 -- not an asteroid (will add it to exclusion list)
19:53:54.33 +38:24:49.8 -- not an asteroid (will add it to exclusion list)
19:39:17.42 +33:45:22.6 -- not an asteroid (will add it to exclusion list)
19:32:32.41 +40:44:53.8 -- not an asteroid (will add it to exclusion list)
20:13:14.72 +34:01:23.3 -- not an asteroid (will add it to exclusion list)
19:50:09.68 +36:46:40.4 -- not an asteroid (will add it to exclusion list)
20:11:14.89 +37:14:20.7 -- not an asteroid (will add it to exclusion list)
19:42:03.54 +34:32:28.8 -- not an asteroid (will add it to exclusion list)
19:24:36.76 +33:42:50.9 -- not an asteroid (will add it to exclusion list)
20:02:37.25 +36:34:49.4 -- not an asteroid (will add it to exclusion list)
19:37:02.54 +34:03:10.0 -- not an asteroid (will add it to exclusion list)
19:52:36.92 +38:35:11.7 -- not an asteroid (will add it to exclusion list)
19:34:46.33 +35:13:28.8 -- not an asteroid (will add it to exclusion list)
19:34:32.40 +33:41:24.7 -- not an asteroid (will add it to exclusion list)
19:40:33.41 +36:40:22.5 -- not an asteroid (will add it to exclusion list)
20:07:32.70 +37:21:45.7 -- not an asteroid (will add it to exclusion list)
19:40:58.96 +36:43:28.6 -- not an asteroid (will add it to exclusion list)
19:56:36.08 +37:05:23.9 -- not an asteroid (will add it to exclusion list)
20:05:37.09 +34:53:31.4 -- not an asteroid (will add it to exclusion list)
19:01:43.19 +35:13:38.2 -- not an asteroid (will add it to exclusion list)
19:49:50.58 +35:20:40.7 -- not an asteroid (will add it to exclusion list)
20:02:24.23 +35:48:38.8 -- not an asteroid (will add it to exclusion list)
20:02:53.78 +40:30:18.2 -- not an asteroid (will add it to exclusion list)
19:40:09.53 +36:00:27.7 -- not an asteroid (will add it to exclusion list)
19:58:23.20 +35:34:15.1 -- not an asteroid (will add it to exclusion list)
20:01:57.03 +35:33:03.8 -- not an asteroid (will add it to exclusion list)
19:50:52.85 +37:40:46.6 -- not an asteroid (will add it to exclusion list)
19:40:41.68 +34:03:15.2 -- not an asteroid (will add it to exclusion list)
19:06:04.52 +35:56:17.0 -- not an asteroid (will add it to exclusion list)
19:46:42.35 +34:50:39.0 -- not an asteroid (will add it to exclusion list)
20:08:06.48 +35:47:53.8 -- not an asteroid (will add it to exclusion list)
19:29:05.69 +37:47:19.7 -- not an asteroid (will add it to exclusion list)
19:59:16.30 +36:50:00.8 -- not an asteroid (will add it to exclusion list)
20:11:54.95 +34:24:07.7 -- not an asteroid (will add it to exclusion list)
19:50:33.34 +34:32:01.5 -- not an asteroid (will add it to exclusion list)
19:44:32.46 +37:10:01.4 -- not an asteroid (will add it to exclusion list)
19:32:23.66 +35:30:26.1 -- not an asteroid (will add it to exclusion list)
19:42:20.33 +37:28:13.6 -- not an asteroid (will add it to exclusion list)
20:01:44.11 +37:27:42.1 -- not an asteroid (will add it to exclusion list)
19:45:25.74 +40:15:37.2 -- not an asteroid (will add it to exclusion list)
20:04:07.76 +39:37:20.2 -- not an asteroid (will add it to exclusion list)
19:42:08.24 +33:23:39.3 -- not an asteroid (will add it to exclusion list)
19:25:28.56 +36:01:04.3 -- not an asteroid (will add it to exclusion list)
19:50:43.13 +33:21:10.6 -- not an asteroid (will add it to exclusion list)
19:41:07.44 +36:43:09.4 -- not an asteroid (will add it to exclusion list)
19:56:28.16 +34:10:44.7 -- not an asteroid (will add it to exclusion list)
20:08:11.42 +35:36:05.2 -- not an asteroid (will add it to exclusion list)
20:13:19.41 +32:57:25.2 -- not an asteroid (will add it to exclusion list)
19:19:30.98 +33:27:37.3 -- not an asteroid (will add it to exclusion list)
19:54:07.89 +40:40:38.8 -- not an asteroid (will add it to exclusion list)
19:58:40.84 +34:45:40.2 -- not an asteroid (will add it to exclusion list)
19:37:49.36 +33:23:19.3 -- not an asteroid (will add it to exclusion list)
19:52:22.24 +38:58:40.0 -- not an asteroid (will add it to exclusion list)
19:48:18.95 +36:57:05.2 -- not an asteroid (will add it to exclusion list)
20:11:21.50 +34:45:58.9 -- not an asteroid (will add it to exclusion list)
19:51:58.84 +34:54:01.1 -- not an asteroid (will add it to exclusion list)
19:24:26.79 +35:11:09.3 -- not an asteroid (will add it to exclusion list)
19:44:09.66 +36:35:55.6 -- not an asteroid (will add it to exclusion list)
19:36:41.76 +36:22:30.5 -- not an asteroid (will add it to exclusion list)
19:47:41.68 +34:35:58.7 -- not an asteroid (will add it to exclusion list)
19:28:16.60 +33:36:44.6 -- not an asteroid (will add it to exclusion list)
19:58:33.06 +37:03:11.2 -- not an asteroid (will add it to exclusion list)
20:05:39.41 +34:15:17.4 -- not an asteroid (will add it to exclusion list)
19:02:40.40 +35:38:22.2 -- not an asteroid (will add it to exclusion list)
19:37:55.01 +40:11:46.3 -- not an asteroid (will add it to exclusion list)
19:52:53.57 +41:30:04.1 -- not an asteroid (will add it to exclusion list)
19:31:29.11 +34:31:59.9 -- not an asteroid (will add it to exclusion list)
19:45:17.12 +39:30:34.5 -- not an asteroid (will add it to exclusion list)
20:12:02.14 +34:43:30.1 -- not an asteroid (will add it to exclusion list)
19:59:29.20 +35:36:14.1 -- not an asteroid (will add it to exclusion list)
19:36:38.89 +37:55:58.0 -- not an asteroid (will add it to exclusion list)
19:27:10.56 +33:18:05.2 -- not an asteroid (will add it to exclusion list)
19:42:39.47 +35:17:05.2 -- not an asteroid (will add it to exclusion list)
19:40:55.93 +34:31:40.8 -- not an asteroid (will add it to exclusion list)
20:15:39.34 +38:25:40.6 -- not an asteroid (will add it to exclusion list)
19:41:55.32 +33:04:20.9 -- not an asteroid (will add it to exclusion list)
19:28:16.85 +33:01:14.5 -- not an asteroid (will add it to exclusion list)
19:47:49.78 +34:14:41.7 -- not an asteroid (will add it to exclusion list)
20:01:50.40 +36:00:49.9 -- not an asteroid (will add it to exclusion list)
19:59:53.44 +36:16:36.1 -- not an asteroid (will add it to exclusion list)
19:31:51.32 +42:45:04.1 -- not an asteroid (will add it to exclusion list)
20:08:30.09 +34:31:54.6 -- not an asteroid (will add it to exclusion list)
19:34:27.81 +37:00:51.6 -- not an asteroid (will add it to exclusion list)
20:03:03.23 +41:08:19.0 -- not an asteroid (will add it to exclusion list)
19:43:08.78 +41:34:10.0 -- not an asteroid (will add it to exclusion list)
20:04:22.43 +36:08:42.3 -- not an asteroid (will add it to exclusion list)
19:48:35.46 +40:26:50.3 -- not an asteroid (will add it to exclusion list)
19:38:56.08 +37:26:01.3 -- not an asteroid (will add it to exclusion list)
19:51:17.64 +33:30:38.4 -- not an asteroid (will add it to exclusion list)
19:34:28.39 +34:43:07.9 -- not an asteroid (will add it to exclusion list)
20:14:53.18 +35:43:57.8 -- not an asteroid (will add it to exclusion list)
19:56:01.49 +39:43:10.7 -- not an asteroid (will add it to exclusion list)
19:45:16.60 +33:06:50.6 -- not an asteroid (will add it to exclusion list)
19:34:53.84 +39:18:12.4 -- not an asteroid (will add it to exclusion list)
19:52:37.87 +36:57:45.7 -- not an asteroid (will add it to exclusion list)
19:51:20.58 +37:18:28.9 -- not an asteroid (will add it to exclusion list)
19:41:53.20 +37:00:31.6 -- not an asteroid (will add it to exclusion list)
19:10:05.83 +37:30:27.8 -- not an asteroid (will add it to exclusion list)
20:03:10.21 +38:17:20.8 -- not an asteroid (will add it to exclusion list)
19:19:53.30 +34:10:46.3 -- not an asteroid (will add it to exclusion list)
20:09:46.62 +38:24:41.3 -- not an asteroid (will add it to exclusion list)
19:42:38.13 +33:55:56.9 -- not an asteroid (will add it to exclusion list)
19:40:32.32 +35:50:48.9 -- not an asteroid (will add it to exclusion list)
19:50:53.66 +37:13:54.2 -- not an asteroid (will add it to exclusion list)
20:02:21.44 +38:21:04.3 -- not an asteroid (will add it to exclusion list)
20:00:23.29 +35:57:25.7 -- not an asteroid (will add it to exclusion list)
19:33:40.81 +33:11:57.9 -- not an asteroid (will add it to exclusion list)
20:00:13.07 +36:03:28.3 -- not an asteroid (will add it to exclusion list)
20:13:03.57 +34:41:39.5 -- not an asteroid (will add it to exclusion list)
20:10:08.56 +33:55:27.1 -- not an asteroid (will add it to exclusion list)
19:08:09.60 +35:40:03.4 -- not an asteroid (will add it to exclusion list)
19:27:01.76 +35:35:31.4 -- not an asteroid (will add it to exclusion list)
19:07:49.10 +36:23:06.5 -- not an asteroid (will add it to exclusion list)
20:05:00.74 +34:45:07.5 -- not an asteroid (will add it to exclusion list)
19:47:56.92 +36:39:51.6 -- not an asteroid (will add it to exclusion list)
20:10:33.86 +33:27:23.6 -- not an asteroid (will add it to exclusion list)
19:59:10.82 +33:23:37.8 -- not an asteroid (will add it to exclusion list)
19:49:43.36 +42:12:13.6 -- not an asteroid (will add it to exclusion list)
20:14:37.70 +35:26:28.2 -- not an asteroid (will add it to exclusion list)
19:35:24.79 +36:39:08.2 -- not an asteroid (will add it to exclusion list)
20:01:57.94 +39:21:10.0 -- not an asteroid (will add it to exclusion list)
19:49:04.87 +36:43:59.5 -- not an asteroid (will add it to exclusion list)
20:01:50.42 +36:49:15.4 -- not an asteroid (will add it to exclusion list)
20:03:18.43 +35:07:54.8 -- not an asteroid (will add it to exclusion list)
19:31:55.38 +33:29:44.6 -- not an asteroid (will add it to exclusion list)
20:01:09.67 +34:01:18.2 -- not an asteroid (will add it to exclusion list)
19:45:50.57 +35:34:08.3 -- not an asteroid (will add it to exclusion list)
19:50:07.56 +33:20:57.0 -- not an asteroid (will add it to exclusion list)
20:12:08.19 +35:56:12.0 -- not an asteroid (will add it to exclusion list)
19:44:24.92 +33:18:28.5 -- not an asteroid (will add it to exclusion list)
20:12:06.16 +34:38:32.5 -- not an asteroid (will add it to exclusion list)
19:46:40.53 +33:53:54.5 -- not an asteroid (will add it to exclusion list)
19:46:36.21 +34:21:31.3 -- not an asteroid (will add it to exclusion list)
20:02:33.70 +34:22:12.1 -- not an asteroid (will add it to exclusion list)
20:16:13.52 +38:36:52.0 -- not an asteroid (will add it to exclusion list)
19:52:24.44 +33:15:03.8 -- not an asteroid (will add it to exclusion list)
19:37:51.16 +34:31:20.9 -- not an asteroid (will add it to exclusion list)
19:44:19.77 +39:52:58.3 -- not an asteroid (will add it to exclusion list)
19:54:23.41 +34:04:49.3 -- not an asteroid (will add it to exclusion list)
20:13:00.23 +33:23:50.4 -- not an asteroid (will add it to exclusion list)
20:04:24.21 +37:07:17.9 -- not an asteroid (will add it to exclusion list)
20:10:35.81 +35:41:49.1 -- not an asteroid (will add it to exclusion list)
19:49:06.09 +36:50:52.9 -- not an asteroid (will add it to exclusion list)
19:55:23.65 +39:12:55.7 -- not an asteroid (will add it to exclusion list)
19:50:43.26 +35:26:56.2 -- not an asteroid (will add it to exclusion list)
19:43:55.09 +40:06:36.6 -- not an asteroid (will add it to exclusion list)
19:31:10.45 +33:34:59.6 -- not an asteroid (will add it to exclusion list)
19:54:49.40 +35:55:51.9 -- not an asteroid (will add it to exclusion list)
20:01:47.38 +40:46:02.4 -- not an asteroid (will add it to exclusion list)
20:06:10.97 +33:36:22.9 -- not an asteroid (will add it to exclusion list)
20:02:56.80 +38:07:46.7 -- not an asteroid (will add it to exclusion list)
19:45:06.97 +38:47:03.3 -- not an asteroid (will add it to exclusion list)
19:50:45.11 +35:11:04.8 -- not an asteroid (will add it to exclusion list)
19:49:34.33 +34:00:11.5 -- not an asteroid (will add it to exclusion list)
19:01:42.64 +42:17:10.4 -- not an asteroid (will add it to exclusion list)
20:03:53.45 +33:46:55.1 -- not an asteroid (will add it to exclusion list)
20:11:08.02 +39:06:50.7 -- not an asteroid (will add it to exclusion list)
20:15:51.65 +38:51:09.3 -- not an asteroid (will add it to exclusion list)
20:12:41.27 +36:27:05.4 -- not an asteroid (will add it to exclusion list)
20:09:15.19 +37:01:43.8 -- not an asteroid (will add it to exclusion list)
19:27:31.48 +39:33:57.9 -- not an asteroid (will add it to exclusion list)
19:30:48.02 +38:57:28.2 -- not an asteroid (will add it to exclusion list)
19:42:06.64 +38:03:33.7 -- not an asteroid (will add it to exclusion list)
20:03:29.86 +40:34:26.9 -- not an asteroid (will add it to exclusion list)
20:02:39.75 +36:36:38.5 -- not an asteroid (will add it to exclusion list)
20:14:04.75 +40:12:40.2 -- not an asteroid (will add it to exclusion list)
19:05:48.27 +33:36:30.3 -- not an asteroid (will add it to exclusion list)
19:44:27.15 +34:19:42.0 -- not an asteroid (will add it to exclusion list)
19:46:18.51 +35:03:46.6 -- not an asteroid (will add it to exclusion list)
20:06:27.19 +40:08:48.0 -- not an asteroid (will add it to exclusion list)
19:45:40.65 +42:35:22.7 -- not an asteroid (will add it to exclusion list)
20:00:29.30 +36:46:08.9 -- not an asteroid (will add it to exclusion list)
19:54:33.29 +38:14:44.8 -- not an asteroid (will add it to exclusion list)
19:57:40.90 +36:01:14.2 -- not an asteroid (will add it to exclusion list)
19:57:58.89 +34:12:52.5 -- not an asteroid (will add it to exclusion list)
20:03:01.62 +34:05:05.8 -- not an asteroid (will add it to exclusion list)
20:13:01.79 +33:26:44.4 -- not an asteroid (will add it to exclusion list)
20:10:00.43 +36:51:09.2 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
19:01:42.64 +42:17:10.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:01:43.19 +35:13:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:02:40.40 +35:38:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:03:58.01 +36:45:27.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:05:01.07 +35:01:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:05:45.47 +37:04:10.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:05:48.27 +33:36:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:06:04.52 +35:56:17.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:49.10 +36:23:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:09.60 +35:40:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:14.40 +42:06:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:09:08.22 +34:26:58.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:10:05.83 +37:30:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:10:17.36 +34:22:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:12:08.80 +37:18:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:15:50.47 +36:32:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:16:12.76 +33:08:41.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:19:10.76 +35:18:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:19:30.98 +33:27:37.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:19:53.30 +34:10:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:23:19.20 +35:01:44.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:24:26.79 +35:11:09.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:24:36.76 +33:42:50.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:24:57.98 +36:12:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:25:00.07 +37:54:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:25:05.42 +33:06:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:25:28.56 +36:01:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:27:01.76 +35:35:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:27:10.56 +33:18:05.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:27:31.48 +39:33:57.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:27:35.37 +34:49:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:28:16.60 +33:36:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:28:16.85 +33:01:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:29:05.69 +37:47:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:29:08.06 +40:44:41.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:29:44.02 +33:10:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:30:39.54 +36:50:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:30:48.02 +38:57:28.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:30:59.97 +35:48:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:31:06.87 +33:07:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:31:10.45 +33:34:59.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:31:29.11 +34:31:59.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:31:51.32 +42:45:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:31:55.38 +33:29:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:32:23.66 +35:30:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:32:32.41 +40:44:53.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:33:40.81 +33:11:57.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:34:27.81 +37:00:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:34:28.39 +34:43:07.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:34:32.40 +33:41:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:34:44.72 +34:13:09.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:34:45.43 +35:14:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:34:46.33 +35:13:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:34:53.84 +39:18:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:35:21.60 +36:04:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:35:24.79 +36:39:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:35:53.60 +36:36:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:36:38.89 +37:55:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:36:41.76 +36:22:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:36:58.41 +33:22:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:37:02.54 +34:03:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:37:09.26 +37:54:12.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:37:49.36 +33:23:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:37:51.16 +34:31:20.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:37:55.01 +40:11:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:38:19.96 +40:52:42.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:38:56.08 +37:26:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:39:17.42 +33:45:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:40:09.53 +36:00:27.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:40:24.09 +41:51:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:40:32.32 +35:50:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:40:33.41 +36:40:22.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:40:41.68 +34:03:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:40:43.02 +36:13:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:40:55.93 +34:31:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:40:58.96 +36:43:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:41:07.44 +36:43:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:41:31.00 +40:00:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:41:46.32 +33:01:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:41:53.20 +37:00:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:41:55.32 +33:04:20.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:42:00.95 +38:11:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:42:03.54 +34:32:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:42:06.64 +38:03:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:42:08.24 +33:23:39.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:42:14.32 +33:59:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:42:20.33 +37:28:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:42:38.13 +33:55:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:42:39.47 +35:17:05.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:42:56.07 +32:55:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:42:56.08 +37:41:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:42:56.73 +34:44:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:43:08.78 +41:34:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:43:31.05 +38:33:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:43:54.51 +38:26:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:43:55.09 +40:06:36.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:43:59.10 +34:01:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:44:03.16 +36:09:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:44:09.66 +36:35:55.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:44:11.71 +40:27:11.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:44:19.77 +39:52:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:44:23.24 +33:24:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:44:24.92 +33:18:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:44:26.98 +35:50:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:44:27.15 +34:19:42.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:44:32.46 +37:10:01.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:45:06.97 +38:47:03.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:45:16.60 +33:06:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:45:16.98 +38:16:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:45:17.12 +39:30:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:45:25.74 +40:15:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:45:40.65 +42:35:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:45:50.57 +35:34:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:46:18.51 +35:03:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:46:36.21 +34:21:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:46:40.53 +33:53:54.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:46:42.35 +34:50:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:46:47.18 +36:57:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:46:55.55 +34:23:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:47:05.35 +37:55:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:47:28.83 +39:09:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:47:29.81 +34:50:04.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:47:41.68 +34:35:58.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:47:46.36 +34:42:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:47:48.48 +36:19:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:47:49.78 +34:14:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:47:56.92 +36:39:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:48:00.70 +33:46:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:48:00.72 +36:25:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:48:18.95 +36:57:05.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:48:26.68 +42:47:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:48:27.84 +39:16:33.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:48:35.46 +40:26:50.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:48:45.74 +34:21:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:48:57.84 +33:11:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:49:04.87 +36:43:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:49:06.09 +36:50:52.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:49:34.33 +34:00:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:49:43.36 +42:12:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:49:50.41 +33:33:37.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:49:50.58 +35:20:40.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:50:07.56 +33:20:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:50:09.68 +36:46:40.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:50:20.66 +36:11:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:50:21.35 +33:31:37.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:50:33.34 +34:32:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:50:40.36 +39:25:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:50:43.13 +33:21:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:50:43.26 +35:26:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:50:45.11 +35:11:04.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:50:52.85 +37:40:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:50:53.66 +37:13:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:51:00.93 +36:24:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:51:17.64 +33:30:38.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:51:20.58 +37:18:28.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:51:33.52 +40:39:37.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:51:58.84 +34:54:01.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:52:09.66 +38:58:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:52:22.24 +38:58:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:52:24.44 +33:15:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:52:33.75 +33:29:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:52:36.27 +37:50:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:52:36.92 +38:35:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:52:37.87 +36:57:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:52:51.63 +39:43:22.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:52:53.57 +41:30:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:53:32.84 +37:51:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:53:40.69 +34:47:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:53:54.33 +38:24:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:54:07.89 +40:40:38.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:54:12.51 +37:52:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:54:23.41 +34:04:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:54:33.29 +38:14:44.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:54:49.40 +35:55:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:55:13.31 +39:33:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:55:19.52 +41:32:17.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:55:23.65 +39:12:55.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:55:53.73 +34:10:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:55:55.49 +36:03:07.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:01.49 +39:43:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:28.16 +34:10:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:32.48 +38:50:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:36.08 +37:05:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:56:42.03 +37:00:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:40.90 +36:01:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:57:58.89 +34:12:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:23.20 +35:34:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:33.06 +37:03:11.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:58:40.84 +34:45:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:10.82 +33:23:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:16.30 +36:50:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:29.20 +35:36:14.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:47.81 +33:23:42.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:59:53.44 +36:16:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:09.09 +39:24:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:13.07 +36:03:28.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:23.29 +35:57:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:29.30 +36:46:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:00:43.13 +40:38:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:09.67 +34:01:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:23.13 +40:06:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:44.11 +37:27:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:47.38 +40:46:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:50.40 +36:00:49.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:50.42 +36:49:15.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:57.03 +35:33:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:01:57.94 +39:21:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:02:21.44 +38:21:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:02:24.23 +35:48:38.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:02:29.79 +37:05:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:02:33.70 +34:22:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:02:35.01 +36:25:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:02:37.25 +36:34:49.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:02:37.35 +35:20:13.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:02:39.75 +36:36:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:02:53.78 +40:30:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:02:56.80 +38:07:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:03:01.62 +34:05:05.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:03:03.23 +41:08:19.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:03:04.91 +37:32:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:03:10.21 +38:17:20.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:03:18.43 +35:07:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:03:29.86 +40:34:26.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:03:33.00 +35:56:57.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:03:35.80 +37:35:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:03:53.28 +39:52:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:03:53.45 +33:46:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:03:58.64 +38:25:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:04:07.76 +39:37:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:04:22.09 +41:02:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:04:22.43 +36:08:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:04:24.21 +37:07:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:05:00.74 +34:45:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:05:30.72 +37:39:35.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:05:37.09 +34:53:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:05:39.41 +34:15:17.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:05:43.79 +40:04:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:06:01.25 +37:14:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:06:06.18 +39:09:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:06:10.97 +33:36:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:06:27.19 +40:08:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:07:32.70 +37:21:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:08:06.48 +35:47:53.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:08:11.42 +35:36:05.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:08:30.09 +34:31:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:08:49.21 +39:04:25.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:08:49.80 +35:30:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:09:08.99 +33:27:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:09:15.19 +37:01:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:09:46.62 +38:24:41.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:10:00.43 +36:51:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:10:08.56 +33:55:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:10:33.86 +33:27:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:10:35.81 +35:41:49.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:11:08.02 +39:06:50.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:11:14.89 +37:14:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:11:21.50 +34:45:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:11:23.75 +38:17:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:11:23.97 +37:54:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:11:49.26 +32:48:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:11:54.95 +34:24:07.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:11:58.84 +33:47:59.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:12:02.14 +34:43:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:12:06.16 +34:38:32.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:12:06.40 +35:03:11.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:12:06.60 +36:24:46.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:12:08.19 +35:56:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:12:10.83 +39:26:10.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:12:24.05 +37:19:53.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:12:32.34 +37:01:28.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:12:36.83 +34:24:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:12:41.27 +36:27:05.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:12:41.82 +33:00:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:12:45.35 +33:25:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:12:50.30 +35:19:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:12:56.06 +32:57:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:13:00.23 +33:23:50.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:13:01.79 +33:26:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:13:03.57 +34:41:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:13:11.69 +41:27:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
20:13:13.24 +33:17:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:13:13.78 +35:42:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:13:14.72 +34:01:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:13:19.41 +32:57:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:13:21.17 +33:02:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
20:13:24.65 +33:11:31.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:13:25.78 +32:55:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
20:13:30.20 +33:53:36.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:14:04.75 +40:12:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:14:09.86 +37:43:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:14:21.18 +36:09:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:14:28.93 +35:06:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:14:32.40 +39:33:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:14:37.70 +35:26:28.2 -- does not seem to be a hot pixel (will add it to exclusion list)
20:14:40.17 +36:35:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
20:14:53.18 +35:43:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:39.34 +38:25:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:50.05 +39:06:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:15:51.65 +38:51:09.3 -- does not seem to be a hot pixel (will add it to exclusion list)
20:16:13.52 +38:36:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
20:16:18.55 +37:55:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
20:17:30.70 +38:28:42.8 -- does not seem to be a hot pixel (will add it to exclusion list)
20:19:30.95 +41:58:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
19:01:42.64 +42:17:10.4 -- not a known variable star
19:01:43.19 +35:13:38.2 -- not a known variable star
19:02:40.40 +35:38:22.2 -- a known variable star
19:03:58.01 +36:45:27.7 -- a known variable star
19:05:01.07 +35:01:55.7 -- not a known variable star
19:05:45.47 +37:04:10.9 -- not a known variable star
19:05:48.27 +33:36:30.3 -- a known variable star
19:06:04.52 +35:56:17.0 -- not a known variable star
19:07:49.10 +36:23:06.5 -- a known variable star
19:08:09.60 +35:40:03.4 -- a known variable star
19:08:14.40 +42:06:33.5 -- a known variable star
19:09:08.22 +34:26:58.1 -- a known variable star
19:10:05.83 +37:30:27.8 -- a known variable star
19:10:17.36 +34:22:33.3 -- not a known variable star
19:12:08.80 +37:18:22.2 -- not a known variable star
19:15:50.47 +36:32:20.7 -- a known variable star
19:16:12.76 +33:08:41.0 -- a known variable star
19:19:10.76 +35:18:03.3 -- not a known variable star
19:19:30.98 +33:27:37.3 -- a known variable star
19:19:53.30 +34:10:46.3 -- a known variable star
19:23:19.20 +35:01:44.8 -- a known variable star
19:24:26.79 +35:11:09.3 -- a known variable star
19:24:36.76 +33:42:50.9 -- not a known variable star
19:24:57.98 +36:12:55.7 -- a known variable star
19:25:00.07 +37:54:05.5 -- a known variable star
19:25:05.42 +33:06:29.5 -- a known variable star
19:25:28.56 +36:01:04.3 -- a known variable star
19:27:01.76 +35:35:31.4 -- a known variable star
19:27:10.56 +33:18:05.2 -- a known variable star
19:27:31.48 +39:33:57.9 -- a known variable star
19:27:35.37 +34:49:30.0 -- a known variable star
19:28:16.60 +33:36:44.6 -- a known variable star
19:28:16.85 +33:01:14.5 -- a known variable star
19:29:05.69 +37:47:19.7 -- a known variable star
19:29:08.06 +40:44:41.8 -- a known variable star
19:29:44.02 +33:10:32.7 -- a known variable star
19:30:39.54 +36:50:05.9 -- a known variable star
19:30:48.02 +38:57:28.2 -- not a known variable star
19:30:59.97 +35:48:34.2 -- a known variable star
19:31:06.87 +33:07:12.0 -- a known variable star
19:31:10.45 +33:34:59.6 -- a known variable star
19:31:29.11 +34:31:59.9 -- not a known variable star
19:31:51.32 +42:45:04.1 -- a known variable star
19:31:55.38 +33:29:44.6 -- not a known variable star
19:32:23.66 +35:30:26.1 -- a known variable star
19:32:32.41 +40:44:53.8 -- a known variable star
19:33:40.81 +33:11:57.9 -- a known variable star
19:34:27.81 +37:00:51.6 -- a known variable star
19:34:28.39 +34:43:07.9 -- a known variable star
19:34:32.40 +33:41:24.7 -- not a known variable star
19:34:44.72 +34:13:09.0 -- not a known variable star
19:34:45.43 +35:14:13.2 -- a known variable star
19:34:46.33 +35:13:28.8 -- a known variable star
19:34:53.84 +39:18:12.4 -- not a known variable star
19:35:21.60 +36:04:03.3 -- a known variable star
19:35:24.79 +36:39:08.2 -- a known variable star
19:35:53.60 +36:36:54.9 -- a known variable star
19:36:38.89 +37:55:58.0 -- a known variable star
19:36:41.76 +36:22:30.5 -- a known variable star
19:36:58.41 +33:22:26.4 -- a known variable star
19:37:02.54 +34:03:10.0 -- a known variable star
19:37:09.26 +37:54:12.6 -- not a known variable star
19:37:49.36 +33:23:19.3 -- a known variable star
19:37:51.16 +34:31:20.9 -- a known variable star
19:37:55.01 +40:11:46.3 -- a known variable star
19:38:19.96 +40:52:42.8 -- not a known variable star
19:38:56.08 +37:26:01.3 -- not a known variable star
19:39:17.42 +33:45:22.6 -- not a known variable star
19:40:09.53 +36:00:27.7 -- a known variable star
19:40:24.09 +41:51:45.0 -- not a known variable star
19:40:32.32 +35:50:48.9 -- not a known variable star
19:40:33.41 +36:40:22.5 -- a known variable star
19:40:41.68 +34:03:15.2 -- a known variable star
19:40:43.02 +36:13:35.1 -- a known variable star
19:40:55.93 +34:31:40.8 -- a known variable star
19:40:58.96 +36:43:28.6 -- a known variable star
19:41:07.44 +36:43:09.4 -- a known variable star
19:41:31.00 +40:00:51.3 -- a known variable star
19:41:46.32 +33:01:18.2 -- a known variable star
19:41:53.20 +37:00:31.6 -- a known variable star
19:41:55.32 +33:04:20.9 -- a known variable star
19:42:00.95 +38:11:33.7 -- a known variable star
19:42:03.54 +34:32:28.8 -- a known variable star
19:42:06.64 +38:03:33.7 -- a known variable star
19:42:08.24 +33:23:39.3 -- a known variable star
19:42:14.32 +33:59:33.8 -- a known variable star
19:42:20.33 +37:28:13.6 -- a known variable star
19:42:38.13 +33:55:56.9 -- a known variable star
19:42:39.47 +35:17:05.2 -- not a known variable star
19:42:56.07 +32:55:33.7 -- a known variable star
19:42:56.08 +37:41:58.7 -- not a known variable star
19:42:56.73 +34:44:58.0 -- a known variable star
19:43:08.78 +41:34:10.0 -- a known variable star
19:43:31.05 +38:33:51.2 -- a known variable star
19:43:54.51 +38:26:44.6 -- a known variable star
19:43:55.09 +40:06:36.6 -- not a known variable star
19:43:59.10 +34:01:50.6 -- not a known variable star
19:44:03.16 +36:09:46.1 -- not a known variable star
19:44:09.66 +36:35:55.6 -- a known variable star
19:44:11.71 +40:27:11.1 -- not a known variable star
19:44:19.77 +39:52:58.3 -- a known variable star
19:44:23.24 +33:24:50.6 -- a known variable star
19:44:24.92 +33:18:28.5 -- a known variable star
19:44:26.98 +35:50:28.5 -- not a known variable star
19:44:27.15 +34:19:42.0 -- not a known variable star
19:44:32.46 +37:10:01.4 -- a known variable star
19:45:06.97 +38:47:03.3 -- a known variable star
19:45:16.60 +33:06:50.6 -- a known variable star
19:45:16.98 +38:16:31.3 -- a known variable star
19:45:17.12 +39:30:34.5 -- not a known variable star
19:45:25.74 +40:15:37.2 -- a known variable star
19:45:40.65 +42:35:22.7 -- a known variable star
19:45:50.57 +35:34:08.3 -- not a known variable star
19:46:18.51 +35:03:46.6 -- a known variable star
19:46:36.21 +34:21:31.3 -- a known variable star
19:46:40.53 +33:53:54.5 -- a known variable star
19:46:42.35 +34:50:39.0 -- a known variable star
19:46:47.18 +36:57:31.1 -- a known variable star
19:46:55.55 +34:23:34.4 -- a known variable star
19:47:05.35 +37:55:42.3 -- a known variable star
19:47:28.83 +39:09:58.6 -- a known variable star
19:47:29.81 +34:50:04.7 -- a known variable star
19:47:41.68 +34:35:58.7 -- a known variable star
19:47:46.36 +34:42:07.2 -- a known variable star
19:47:48.48 +36:19:12.9 -- not a known variable star
19:47:49.78 +34:14:41.7 -- a known variable star
19:47:56.92 +36:39:51.6 -- a known variable star
19:48:00.70 +33:46:05.9 -- a known variable star
19:48:00.72 +36:25:50.5 -- a known variable star
19:48:18.95 +36:57:05.2 -- a known variable star
19:48:26.68 +42:47:33.0 -- a known variable star
19:48:27.84 +39:16:33.9 -- a known variable star
19:48:35.46 +40:26:50.3 -- a known variable star
19:48:45.74 +34:21:55.1 -- a known variable star
19:48:57.84 +33:11:30.0 -- not a known variable star
19:49:04.87 +36:43:59.5 -- a known variable star
19:49:06.09 +36:50:52.9 -- a known variable star
19:49:34.33 +34:00:11.5 -- a known variable star
19:49:43.36 +42:12:13.6 -- a known variable star
19:49:50.41 +33:33:37.1 -- a known variable star
19:49:50.58 +35:20:40.7 -- not a known variable star
19:50:07.56 +33:20:57.0 -- a known variable star
19:50:09.68 +36:46:40.4 -- a known variable star
19:50:20.66 +36:11:06.2 -- a known variable star
19:50:21.35 +33:31:37.0 -- a known variable star
19:50:33.34 +34:32:01.5 -- not a known variable star
19:50:40.36 +39:25:24.9 -- a known variable star
19:50:43.13 +33:21:10.6 -- a known variable star
19:50:43.26 +35:26:56.2 -- a known variable star
19:50:45.11 +35:11:04.8 -- a known variable star
19:50:52.85 +37:40:46.6 -- a known variable star
19:50:53.66 +37:13:54.2 -- a known variable star
19:51:00.93 +36:24:04.4 -- a known variable star
19:51:17.64 +33:30:38.4 -- a known variable star
19:51:20.58 +37:18:28.9 -- not a known variable star
19:51:33.52 +40:39:37.4 -- a known variable star
19:51:58.84 +34:54:01.1 -- a known variable star
19:52:09.66 +38:58:20.5 -- not a known variable star
19:52:22.24 +38:58:40.0 -- a known variable star
19:52:24.44 +33:15:03.8 -- a known variable star
19:52:33.75 +33:29:22.1 -- a known variable star
19:52:36.27 +37:50:02.8 -- a known variable star
19:52:36.92 +38:35:11.7 -- a known variable star
19:52:37.87 +36:57:45.7 -- a known variable star
19:52:51.63 +39:43:22.3 -- a known variable star
19:52:53.57 +41:30:04.1 -- a known variable star
19:53:32.84 +37:51:45.6 -- a known variable star
19:53:40.69 +34:47:35.8 -- a known variable star
19:53:54.33 +38:24:49.8 -- a known variable star
19:54:07.89 +40:40:38.8 -- a known variable star
19:54:12.51 +37:52:30.1 -- a known variable star
19:54:23.41 +34:04:49.3 -- a known variable star
19:54:33.29 +38:14:44.8 -- a known variable star
19:54:49.40 +35:55:51.9 -- a known variable star
19:55:13.31 +39:33:00.9 -- a known variable star
19:55:19.52 +41:32:17.4 -- a known variable star
19:55:23.65 +39:12:55.7 -- a known variable star
19:55:53.73 +34:10:49.3 -- a known variable star
19:55:55.49 +36:03:07.9 -- not a known variable star
19:56:01.49 +39:43:10.7 -- a known variable star
19:56:28.16 +34:10:44.7 -- a known variable star
19:56:32.48 +38:50:19.3 -- not a known variable star
19:56:36.08 +37:05:23.9 -- a known variable star
19:56:42.03 +37:00:26.7 -- a known variable star
19:57:40.90 +36:01:14.2 -- not a known variable star
19:57:58.89 +34:12:52.5 -- a known variable star
19:58:23.20 +35:34:15.1 -- a known variable star
19:58:33.06 +37:03:11.2 -- a known variable star
19:58:40.84 +34:45:40.2 -- not a known variable star
19:59:10.82 +33:23:37.8 -- a known variable star
19:59:16.30 +36:50:00.8 -- a known variable star
19:59:29.20 +35:36:14.1 -- a known variable star
19:59:47.81 +33:23:42.6 -- not a known variable star
19:59:53.44 +36:16:36.1 -- a known variable star
20:00:09.09 +39:24:58.8 -- a known variable star
20:00:13.07 +36:03:28.3 -- a known variable star
20:00:23.29 +35:57:25.7 -- a known variable star
20:00:29.30 +36:46:08.9 -- a known variable star
20:00:43.13 +40:38:04.4 -- a known variable star
20:01:09.67 +34:01:18.2 -- a known variable star
20:01:23.13 +40:06:31.5 -- a known variable star
20:01:44.11 +37:27:42.1 -- a known variable star
20:01:47.38 +40:46:02.4 -- a known variable star
20:01:50.40 +36:00:49.9 -- a known variable star
20:01:50.42 +36:49:15.4 -- a known variable star
20:01:57.03 +35:33:03.8 -- a known variable star
20:01:57.94 +39:21:10.0 -- a known variable star
20:02:21.44 +38:21:04.3 -- a known variable star
20:02:24.23 +35:48:38.8 -- a known variable star
20:02:29.79 +37:05:55.9 -- not a known variable star
20:02:33.70 +34:22:12.1 -- a known variable star
20:02:35.01 +36:25:58.2 -- a known variable star
20:02:37.25 +36:34:49.4 -- a known variable star
20:02:37.35 +35:20:13.8 -- not a known variable star
20:02:39.75 +36:36:38.5 -- a known variable star
20:02:53.78 +40:30:18.2 -- a known variable star
20:02:56.80 +38:07:46.7 -- a known variable star
20:03:01.62 +34:05:05.8 -- a known variable star
20:03:03.23 +41:08:19.0 -- a known variable star
20:03:04.91 +37:32:26.1 -- a known variable star
20:03:10.21 +38:17:20.8 -- a known variable star
20:03:18.43 +35:07:54.8 -- a known variable star
20:03:29.86 +40:34:26.9 -- not a known variable star
20:03:33.00 +35:56:57.7 -- a known variable star
20:03:35.80 +37:35:08.9 -- a known variable star
20:03:53.28 +39:52:36.1 -- a known variable star
20:03:53.45 +33:46:55.1 -- a known variable star
20:03:58.64 +38:25:33.2 -- not a known variable star
20:04:07.76 +39:37:20.2 -- a known variable star
20:04:22.09 +41:02:12.9 -- a known variable star
20:04:22.43 +36:08:42.3 -- a known variable star
20:04:24.21 +37:07:17.9 -- a known variable star
20:05:00.74 +34:45:07.5 -- a known variable star
20:05:30.72 +37:39:35.4 -- not a known variable star
20:05:37.09 +34:53:31.4 -- a known variable star
20:05:39.41 +34:15:17.4 -- a known variable star
20:05:43.79 +40:04:30.5 -- not a known variable star
20:06:01.25 +37:14:30.0 -- not a known variable star
20:06:06.18 +39:09:31.3 -- a known variable star
20:06:10.97 +33:36:22.9 -- not a known variable star
20:06:27.19 +40:08:48.0 -- a known variable star
20:07:32.70 +37:21:45.7 -- a known variable star
20:08:06.48 +35:47:53.8 -- a known variable star
20:08:11.42 +35:36:05.2 -- a known variable star
20:08:30.09 +34:31:54.6 -- a known variable star
20:08:49.21 +39:04:25.0 -- a known variable star
20:08:49.80 +35:30:51.7 -- not a known variable star
20:09:08.99 +33:27:24.9 -- not a known variable star
20:09:15.19 +37:01:43.8 -- a known variable star
20:09:46.62 +38:24:41.3 -- not a known variable star
20:10:00.43 +36:51:09.2 -- a known variable star
20:10:08.56 +33:55:27.1 -- not a known variable star
20:10:33.86 +33:27:23.6 -- a known variable star
20:10:35.81 +35:41:49.1 -- a known variable star
20:11:08.02 +39:06:50.7 -- a known variable star
20:11:14.89 +37:14:20.7 -- a known variable star
20:11:21.50 +34:45:58.9 -- a known variable star
20:11:23.75 +38:17:04.3 -- a known variable star
20:11:23.97 +37:54:20.3 -- a known variable star
20:11:49.26 +32:48:37.8 -- not a known variable star
20:11:54.95 +34:24:07.7 -- a known variable star
20:11:58.84 +33:47:59.0 -- a known variable star
20:12:02.14 +34:43:30.1 -- not a known variable star
20:12:06.16 +34:38:32.5 -- a known variable star
20:12:06.40 +35:03:11.6 -- not a known variable star
20:12:06.60 +36:24:46.7 -- a known variable star
20:12:08.19 +35:56:12.0 -- a known variable star
20:12:10.83 +39:26:10.7 -- a known variable star
20:12:24.05 +37:19:53.2 -- not a known variable star
20:12:32.34 +37:01:28.9 -- a known variable star
20:12:36.83 +34:24:11.7 -- not a known variable star
20:12:41.27 +36:27:05.4 -- not a known variable star
20:12:41.82 +33:00:51.7 -- not a known variable star
20:12:45.35 +33:25:41.7 -- not a known variable star
20:12:50.30 +35:19:36.0 -- not a known variable star
20:12:56.06 +32:57:06.9 -- a known variable star
20:13:00.23 +33:23:50.4 -- a known variable star
20:13:01.79 +33:26:44.4 -- a known variable star
20:13:03.57 +34:41:39.5 -- not a known variable star
20:13:11.69 +41:27:21.1 -- a known variable star
20:13:13.24 +33:17:31.6 -- a known variable star
20:13:13.78 +35:42:30.6 -- not a known variable star
20:13:14.72 +34:01:23.3 -- a known variable star
20:13:19.41 +32:57:25.2 -- a known variable star
20:13:21.17 +33:02:49.7 -- a known variable star
20:13:24.65 +33:11:31.4 -- not a known variable star
20:13:25.78 +32:55:18.9 -- a known variable star
20:13:30.20 +33:53:36.3 -- not a known variable star
20:14:04.75 +40:12:40.2 -- a known variable star
20:14:09.86 +37:43:22.2 -- not a known variable star
20:14:21.18 +36:09:56.5 -- not a known variable star
20:14:28.93 +35:06:32.2 -- a known variable star
20:14:32.40 +39:33:17.3 -- not a known variable star
20:14:37.70 +35:26:28.2 -- not a known variable star
20:14:40.17 +36:35:15.5 -- a known variable star
20:14:53.18 +35:43:57.8 -- a known variable star
20:15:39.34 +38:25:40.6 -- a known variable star
20:15:50.05 +39:06:36.4 -- not a known variable star
20:15:51.65 +38:51:09.3 -- a known variable star
20:16:13.52 +38:36:52.0 -- a known variable star
20:16:18.55 +37:55:39.4 -- a known variable star
20:17:30.70 +38:28:42.8 -- not a known variable star
20:19:30.95 +41:58:23.6 -- not a known variable star
Found 74 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
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303 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 303 (excluding asteroids and hot pixels, 74 new), not updating the exclusion list!
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Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
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Positions of planets computed with util/planet_finder/main.py for JD(UT)2461139.80823208 -observatory V36
23:34:08.99 -05:16:46.5 Mercury (0.2mag)
02:36:18.18 +15:11:26.4 Venus (-3.9mag)
23:58:48.19 -01:13:56.1 Mars (1.2mag)
07:09:49.94 +22:50:42.3 Jupiter (-2.1mag)
00:26:10.53 +00:30:08.7 Saturn (0.9mag)
03:46:19.73 +19:43:03.8 Uranus (5.8mag)
00:09:57.10 -00:20:59.4 Neptune (7.8mag)
20:33:25.23 -22:52:26.9 Pluto (14.5mag)
18:44:53.17 -28:01:24.3 Moon (-10.6mag)
-rw-r--r-- 1 apache apache 362 Apr 9 02:26 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461139.80823208:
07:09:57.16 +22:50:28.9 Io (5.7mag)
07:10:00.47 +22:50:22.1 Europa (5.9mag)
07:10:02.97 +22:50:10.1 Ganymede (5.3mag)
07:09:20.40 +22:51:45.4 Callisto (6.5mag)
07:13:26.45 +22:41:35.4 Himalia (15.3mag)
07:09:50.31 +22:50:38.8 Thebe (16.2mag)
07:13:28.68 +23:10:58.5 Elara (17.3mag)
07:08:15.49 +23:34:12.6 Pasiphae (17.4mag)
07:18:18.14 +22:48:00.8 Carme (18.5mag)
00:26:17.72 +00:29:57.9 Titan (8.8mag)
00:26:14.62 +00:30:19.1 Rhea (10.1mag)
00:26:04.00 +00:31:18.9 Iapetus (11.5mag)
00:26:22.24 +00:29:55.3 Hyperion (14.8mag)
00:27:52.53 +00:39:39.1 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 9 02:27 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461139.80823208:
15:04:48.28 -11:06:26.7 JWST
17:49:16.56 +37:50:27.6 Chandra
18:26:21.10 -29:27:54.1 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 9 02:26 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461139.80823208 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:48:52.31 -28:24:04.6 13.9mag P/2010 H2 (Vales)
05:02:06.30 -69:59:18.7 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:31:06.50 +31:23:39.3 17.2mag C/2017 K2 (PANSTARRS)
17:30:53.32 +09:44:50.6 17.6mag C/2021 G2 (ATLAS)
23:08:19.48 +28:58:32.9 17.0mag C/2022 E2 (ATLAS)
04:21:31.21 +25:51:10.8 15.9mag C/2022 N2 (PANSTARRS)
09:02:13.82 +31:57:16.0 16.2mag C/2022 QE78 (ATLAS)
08:30:13.98 -00:52:49.1 17.3mag C/2022 R6 (PANSTARRS)
18:55:06.46 +17:57:50.0 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:42:41.49 -11:37:04.2 17.6mag P/2023 B1 (PANSTARRS)
09:11:01.71 -12:58:39.4 17.6mag C/2023 F3 (ATLAS)
21:47:05.72 +62:31:54.8 17.5mag C/2023 H5 (Lemmon)
19:24:24.26 -03:38:24.0 14.2mag C/2023 R1 (PANSTARRS)
21:41:13.50 +85:00:30.5 17.8mag C/2023 X2 (Lemmon)
06:15:18.70 +63:33:18.0 17.1mag C/2024 A1 (ATLAS)
04:58:24.88 +15:52:07.0 10.6mag C/2024 E1 (Wierzchos)
16:23:21.96 +05:17:26.2 17.4mag C/2024 G6 (ATLAS)
20:18:42.18 +13:29:22.2 14.7mag C/2024 J3 (ATLAS)
03:20:27.00 -23:25:26.7 16.4mag C/2024 T5 (ATLAS)
05:11:10.20 +47:00:00.1 17.7mag C/2025 J1 (Borisov)
14:06:33.02 +40:21:28.0 14.9mag C/2025 L1 (ATLAS)
03:14:58.03 -25:11:54.6 17.8mag C/2025 Q3 (ATLAS)
23:03:18.71 +19:45:55.6 9.6mag C/2025 R3 (PANSTARRS)
12:57:01.95 +02:35:40.3 17.5mag C/2025 Y1 (ATLAS)
02:19:04.22 +03:42:00.9 10.4mag C/2026 A1 (MAPS)
23:40:10.50 +35:54:46.4 14.4mag C/2026 B2 (Sun-Gao)
18:29:53.12 -10:04:02.1 12.2mag 10P/Tempel
15:09:06.24 +03:51:08.8 13.4mag 24P/Schaumasse
11:04:44.92 -01:45:06.8 15.7mag 29P/Schwassmann-Wachmann
17:58:24.86 -09:52:02.0 17.8mag 40P/Vaisala
10:38:14.89 -04:39:45.8 16.8mag 43P/Wolf-Harrington
01:38:20.53 +16:20:17.4 17.2mag 47P/Ashbrook-Jackson
06:58:42.11 +38:25:56.5 17.0mag 63P/Wild
23:20:25.00 -12:15:59.4 15.7mag 65P/Gunn
03:45:39.13 +18:53:20.4 15.9mag 76P/West-Kohoutek-Ikemura
00:50:51.88 +06:54:21.6 14.4mag 78P/Gehrels
22:42:24.36 -11:21:47.8 14.6mag 88P/Howell
01:51:41.86 +18:49:17.5 15.1mag 93P/Lovas
04:42:27.47 +31:54:50.3 16.3mag 123P/West-Hartley
08:20:57.75 +41:27:03.6 16.2mag 124P/Mrkos
02:22:56.63 +13:36:53.6 16.4mag 128P/Shoemaker-Holt
02:34:27.25 +13:39:27.0 17.5mag 131P/Mueller
00:51:32.61 +10:48:44.5 11.0mag 141P/Machholz
01:01:16.01 +02:21:37.8 11.0mag 141P-A/Machholz
23:50:02.45 -01:26:05.5 13.6mag 141P-D/Machholz
01:30:51.64 +04:04:15.4 17.9mag 141P-I/Machholz
00:43:46.20 -04:52:31.5 15.2mag 162P/SidingSpring
10:30:03.83 +31:18:39.2 17.9mag 164P/Christensen
06:24:08.66 +24:26:43.3 17.9mag 198P/ODAS
15:03:17.34 -00:48:44.7 17.4mag 210P/Christensen
21:18:47.73 -13:04:05.4 17.5mag 218P/LINEAR
17:14:12.82 -14:43:17.9 16.2mag 235P/LINEAR
05:20:11.06 +34:08:49.9 16.6mag 240P/NEAT
07:35:26.16 -05:55:03.7 17.7mag 242P/Spahr
15:45:01.24 +06:31:58.8 17.5mag 391P/Kowalski
07:31:50.46 +21:20:04.5 17.6mag 450P/LONEOS
05:26:15.68 +45:25:32.8 17.5mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 9 02:26 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
05:00:45.52 -29:51:06.20 AT2026hvw 2026-04-6.03 16.51
19:49:33.10 -23:37:11.00 ASASSN-26cl 2026-04-5.29 14.98
19:32:43.55 -22:39:33.40 ASASSN-26cm 2026-04-4.3 13.88
18:08:57.38 +76:48:23.60 ASASSN-26ck 2026-04-2.37 15.38
16:16:36.10 +44:52:30.20 AT2026hyy 2026-04-2.58 13.81
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.70 -27:51:49.80 SN2026gvk 2026-03-30 15.48
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.96 -45:55:38.40 ASASSN-26bt 2026-03-18.8 16.32
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.46 +15:42:15.50 SN2026ehe 2026-03-12.34 -0.18
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.33 -37:49:33.00 ASASSN-26bk 2026-03-2.06 13.58
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.29 +19:58:46.30 ASASSN-26be 2026-02-25.56 14.95
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
11:50:37.32 +55:21:13.70 SN 2026dix 2026-02-21.43 16.39
16:21:19.69 -63:47:29.40 ASASSN-26az 2026-02-21.03 17.02
02:45:30.93 -54:17:43.10 SN 2026cju 2026-02-21.04 17.54
01:58:40.68 +47:34:50.10 ASASSN-26av 2026-02-21.09 15.97
18:35:53.01 -42:31:38.90 ASASSN-26aw 2026-02-21.12 15.89
11:40:18.88 -39:45:09.20 ASASSN-26ax 2026-02-21.08 15.73
02:26:23.52 -51:42:29.80 ASASSN-26ay 2026-02-21.04 13.93
08:46:07.66 +01:17:43.90 ASASSN-26ba 2026-02-20.23 15.43
14:15:47.49 -48:05:16.60 SN2026dez 2026-02-19.31 15.91
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.22 -11:25:16.10 AT2026bzh 2026-02-12.16 17.22
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
19:32:43.67 -22:39:30.7 TCP J19324367-2239307 2026-04-05.4395 13.6mag
16:16:36.03 +44:52:28.9 TCP J16163603+4452289 2026-04-05.6655 14.2mag
-rw-r--r-- 1 apache apache 187K Apr 9 02:26 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
17:38:02.570 +25:54:11.91 AT 2026ifx 2026-03-27.88 20.89
16:42:02.490 +40:59:30.50 AT 2026ifw 2026-03-27.86 21.32
16:24:14.050 +39:37:35.59 AT 2026ifv 2026-03-27.86 20.81
16:16:45.660 +38:01:36.33 AT 2026ifu 2026-03-27.86 21.15
16:28:23.190 +36:11:26.67 AT 2026ift 2026-03-27.86 21.53
16:16:10.610 +36:40:26.87 AT 2026ifs 2026-03-27.86 20.03
16:42:08.700 +33:28:34.26 AT 2026ifr 2026-03-27.86 21.24
16:45:41.760 +34:10:06.31 AT 2026ifq 2026-03-27.86 21.64
16:50:17.550 +33:04:52.33 AT 2026ifp 2026-03-27.86 19.99
16:52:21.140 +31:25:32.03 AT 2026ifo 2026-03-27.86 19.73
16:06:48.970 +28:22:45.47 AT 2026ifn 2026-03-27.85 21.37
16:26:20.250 +28:06:35.30 AT 2026ifm 2026-03-27.85 20.13
17:01:36.800 +29:43:13.81 AT 2026ifl 2026-03-27.85 20.62
17:06:26.770 +28:47:25.16 AT 2026ifk 2026-03-27.85 21.39
16:47:18.680 +27:13:25.92 AT 2026ifj 2026-03-27.85 20.26
15:55:49.720 +37:36:32.33 AT 2026ifi 2026-03-24.80 21.32
16:05:53.820 +48:45:26.80 AT 2026ifh 2026-03-23.81 21.26
16:27:03.110 +44:45:26.84 AT 2026ifg 2026-03-23.81 21.9
16:41:17.580 +44:27:03.47 AT 2026iff 2026-03-23.81 22.17
16:30:53.670 +55:47:08.39 AT 2026ife 2026-03-30.85 20.99
-rw-r--r-- 1 apache apache 30K Apr 9 02:26 tns_transients_list.txt
