This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ
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
ATO J284.4121-05.4871,2461140.8405,11.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J284.4121-05.4871 20260410.3405 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
ATO J279.2504-06.2371,2461140.8405,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J279.2504-06.2371 20260410.3405 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
ZTF J185951.76-013501.7,2461140.8405,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J185951.76-013501.7 20260410.3405 13.44CV 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 J283.1905-01.3534,2461140.8405,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J283.1905-01.3534 20260410.3405 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
ASASSN-V J190710.42-010443.6,2461140.8405,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J190710.42-010443.6 20260410.3405 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
target,2461140.8405,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260410.3405 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
Gaia DR3 4267679414587876352,2461140.8405,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 4267679414587876352 20260410.3405 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 J286.6195-02.7351,2461140.8405,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J286.6195-02.7351 20260410.3405 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
ATO J287.1271-00.4507,2461140.8405,12.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J287.1271-00.4507 20260410.3405 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
ATO J285.9455-05.9319,2461140.8405,12.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J285.9455-05.9319 20260410.3405 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
GDS_J1846165-061336,2461140.8405,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J1846165-061336 20260410.3405 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!
TCP 2026 04 10.3405* 18 24 06.80 +01 54 53.7 14.0 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J182406.36+015458.1,2461140.8405,14.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J182406.36+015458.1 20260410.3405 14.02CV 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
NSVS 13954633,2461140.8405,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 13954633 20260410.3405 13.62CV 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
ZTF J190824.56+015747.3,2461140.8405,13.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J190824.56+015747.3 20260410.3405 13.84CV 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
V1549 Aql,2461140.8405,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1549 Aql 20260410.3405 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
GDS_J1840102-060816,2461140.8405,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J1840102-060816 20260410.3405 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J1901413+001420,2461140.8405,13.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J1901413+001420 20260410.3405 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
GDS_J1902143-001908,2461140.8405,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J1902143-001908 20260410.3405 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 4266291830951396224,2461140.8405,13.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4266291830951396224 20260410.3405 13.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J1847266-041313,2461140.8405,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J1847266-041313 20260410.3405 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.3405* 18 27 38.03 -02 35 57.1 12.5 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J1827379-023558,2461140.8405,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J1827379-023558 20260410.3405 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J185328.68+012156.8,2461140.8405,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J185328.68+012156.8 20260410.3405 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J1855486-014554,2461140.8405,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J1855486-014554 20260410.3405 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
GDS_J1829555-055823,2461140.8405,13.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J1829555-055823 20260410.3405 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
GDS_J1846577-041624,2461140.8405,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J1846577-041624 20260410.3405 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
ASASSN-V J185634.12+003515.0,2461140.8405,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J185634.12+003515.0 20260410.3405 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 10.3405* 18 36 24.26 -03 41 32.2 13.2 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J1836241-034131,2461140.8405,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J1836241-034131 20260410.3405 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
NSVS 13957122,2461140.8405,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 13957122 20260410.3405 13.30CV 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
ATO J284.4665+01.3918,2461140.8405,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J284.4665+01.3918 20260410.3405 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
2MASS J19000277-0349075,2461140.8405,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
2MASS J19000277-0349075 20260410.3405 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J190710.42+005135.2,2461140.8405,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J190710.42+005135.2 20260410.3405 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 13962543,2461140.8405,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 13962543 20260410.3405 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
GDS_J1852562-040644,2461140.8405,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J1852562-040644 20260410.3405 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
FASTT 1196,2461140.8405,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
FASTT 1196 20260410.3405 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
2MASS J18504675-0502101,2461140.8405,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J18504675-0502101 20260410.3405 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
ASASSN-V J190135.57-061402.4,2461140.8405,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J190135.57-061402.4 20260410.3405 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
[WLR2013] 26,2461140.8405,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
[WLR2013] 26 20260410.3405 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J190519.28-014219.4,2461140.8405,12.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J190519.28-014219.4 20260410.3405 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
ASASSN-V J190508.39-001134.2,2461140.8405,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J190508.39-001134.2 20260410.3405 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
ASASSN-V J190811.18-052807.3,2461140.8405,13.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J190811.18-052807.3 20260410.3405 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
ATO J286.8793-05.4972,2461140.8405,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J286.8793-05.4972 20260410.3405 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
ASAS J190655-0233.8,2461140.8405,11.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J190655-0233.8 20260410.3405 11.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J1851172-050300,2461140.8405,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J1851172-050300 20260410.3405 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
Gaia DR3 4261377387571018112,2461140.8405,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 4261377387571018112 20260410.3405 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
ZTF J190825.29+002607.1,2461140.8405,13.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J190825.29+002607.1 20260410.3405 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 J287.0504-05.5896,2461140.8405,11.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J287.0504-05.5896 20260410.3405 11.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J190641.16-051324.6,2461140.8405,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J190641.16-051324.6 20260410.3405 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
ASASSN-V J185803.39-034902.3,2461140.8405,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J185803.39-034902.3 20260410.3405 13.07CV 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
NSVS 13949520,2461140.8405,12.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 13949520 20260410.3405 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
NSVS 13953187,2461140.8405,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 13953187 20260410.3405 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
ZTF J190729.02-041630.2,2461140.8405,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J190729.02-041630.2 20260410.3405 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
Gaia DR3 4254075878812964224,2461140.8405,13.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4254075878812964224 20260410.3405 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 13924675,2461140.8405,13.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 13924675 20260410.3405 13.31CV 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
GDS_J1854306-042353,2461140.8405,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J1854306-042353 20260410.3405 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
ASASSN-V J190353.72-034136.9,2461140.8405,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J190353.72-034136.9 20260410.3405 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 4267324268007663744,2461140.8405,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4267324268007663744 20260410.3405 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
NSVS 13983451,2461140.8405,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 13983451 20260410.3405 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
GDS_J1900201-022205,2461140.8405,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J1900201-022205 20260410.3405 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
ASASSN-V J190611.83-043154.0,2461140.8405,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J190611.83-043154.0 20260410.3405 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
ZTF J190312.31-035559.7,2461140.8405,13.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J190312.31-035559.7 20260410.3405 13.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J190900.50-000818.9,2461140.8405,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J190900.50-000818.9 20260410.3405 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
V1793 Aql,2461140.8405,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1793 Aql 20260410.3405 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
NSVS 13955316,2461140.8405,13.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 13955316 20260410.3405 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
GDS_J1851374-032610,2461140.8405,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J1851374-032610 20260410.3405 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 13985056,2461140.8405,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 13985056 20260410.3405 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
GDS_J1852222-043328,2461140.8405,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J1852222-043328 20260410.3405 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 J280.0599-05.7204,2461140.8405,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J280.0599-05.7204 20260410.3405 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 4206253406472481536,2461140.8405,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4206253406472481536 20260410.3405 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
NSVS 13951828,2461140.8405,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 13951828 20260410.3405 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 4206147269239515648,2461140.8405,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4206147269239515648 20260410.3405 11.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 13983865,2461140.8405,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 13983865 20260410.3405 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
GDS_J1843261-051144,2461140.8405,12.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J1843261-051144 20260410.3405 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
VARIABLE_NAME,2461140.8405,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260410.3405 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!
TCP 2026 04 10.3405* 18 30 06.26 +00 42 33.2 13.4 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J183006.17+004233.6,2461140.8405,13.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J183006.17+004233.6 20260410.3405 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
ASASSN-V J190549.60-015157.3,2461140.8405,13.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J190549.60-015157.3 20260410.3405 13.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GDS_J1858104-032641,2461140.8405,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J1858104-032641 20260410.3405 13.07CV 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
NSVS 13963701,2461140.8405,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 13963701 20260410.3405 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
ZTF J190648.37+013013.1,2461140.8405,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J190648.37+013013.1 20260410.3405 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
NSVS 13827995,2461140.8405,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 13827995 20260410.3405 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 J283.3385-01.0944,2461140.8405,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J283.3385-01.0944 20260410.3405 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
GDS_J1850044-053839,2461140.8405,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J1850044-053839 20260410.3405 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J185417.65-052233.1,2461140.8405,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J185417.65-052233.1 20260410.3405 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
NSVS 13958054,2461140.8405,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 13958054 20260410.3405 13.24CV 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
GDS_J1856562-012539,2461140.8405,12.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GDS_J1856562-012539 20260410.3405 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461099.00015142 27.02.2026 12:00:03.083 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
First image: 2461099.00015142 27.02.2026 12:00:03.083 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
Last image: 2461140.84073784 10.04.2026 08:10:29.749 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 72
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.06
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: 7 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): 8851
Objects passed selection criteria: 8840
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 8088.75
Average stars matched: 7847.5 (97.0175 %)
Memory usage VmPeak: 115540 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 Fri Apr 10 04:13:26 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: 2461099.00015142 27.02.2026 12:00:03.083 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
First image: 2461099.00015142 27.02.2026 12:00:03.083 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
Last image: 2461140.84073784 10.04.2026 08:10:29.749 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 446
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.77
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: 56 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): 104186
Objects passed selection criteria: 103937
Measurements per detected object (mean, median, min, max): 3.1 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 3.0 2 4
Average stars detected per image: 87006.8
Average stars matched: 83349.5 (95.7966 %)
Memory usage VmPeak: 1887868 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 Fri Apr 10 04:16:29 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits
SExtractor catalog cache: saved Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat to cache
SExtractor catalog cache: saved Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.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/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.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: 2461140.84018000
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_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits exists and is non-empty
Saving wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits to local_wcs_cache/
'wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits' -> 'local_wcs_cache/wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits'
wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits exists and is non-empty
Saving wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits to local_wcs_cache/
'wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits' -> 'local_wcs_cache/wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits'
wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits exists and is non-empty
Saving wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits to local_wcs_cache/
'wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits' -> 'local_wcs_cache/wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits'
wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits exists and is non-empty
Saving wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits to local_wcs_cache/
'wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits' -> 'local_wcs_cache/wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 18:51:25.226 -01:59:55.32
Second-epoch image center 18:51:41.246 -02:01:00.67
Angular distance between the image centers 0.0691 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 18:51:25.226 -01:59:55.32
Second-epoch image center 18:51:43.130 -02:00:55.44
Angular distance between the image centers 0.0764 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 18:51:41.246 -02:01:00.67
Second-epoch second image center 18:51:43.130 -02:00:55.44
Angular distance between the image centers 0.00798 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/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits &> /tmp/tmp.ahWdGlgxqw
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits &> /tmp/tmp.4UoXxDucUC
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits &> /tmp/tmp.ry02yA6if5
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits &> /tmp/tmp.FDfd2JiF6m
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits
Calibrating the magnitude scale
Found non-empty wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.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_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits and wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.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_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits and wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat
Found non-empty wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits and wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat
The reference image (wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits) and catalog (wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat) found
'wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat' -> 'wcsmag.cat'
Read 13310 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 274.9619 to 290.7764 deg, Dec -7.2966 to +3.2981 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 274.9619 to 290.7764 deg, Dec -7.2966 to 3.2981 deg
Loaded 9541 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): 6890 out of 7408 total matches.
Matched with Tycho-2 7408 out of 13310 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.858998
a=0.000000 b=1.000000 c=22.858998
From vast_summary.log: estimated ref. image limiting mag.: -8.06
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.80
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.80
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 45 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
2.3 pix Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
3.1 pix fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits
3.1 pix fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits
Limiting magnitude estimates:
14.8 mag. Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
14.8 mag. Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
14.0 mag. fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits
14.0 mag. fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 11.6 (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.ahWdGlgxqw (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits' -> 'wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
WCS_IMAGE_NAME=wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
WCS-calibrated image found: wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
Checking if the catalog wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat corresponding to the image wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits alredy exist and is non-empty...
Catalog wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat corresponding to the image wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
WCS catalog name: wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1253, passed=13310
Got 13310 stars (including 12037 good ones) from the SExtractor catalog wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat
util/solve_plate_with_UCAC5 got 13310 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 913 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 12599 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 12599 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 945 matched stars entering correct_measured_positions(), 12598 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 945 stars left (next iteration limit 1039)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits -region wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.4UoXxDucUC (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits' -> 'wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
WCS_IMAGE_NAME=wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
WCS-calibrated image found: wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
Checking if the catalog wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat corresponding to the image wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits alredy exist and is non-empty...
Catalog wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat corresponding to the image wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
WCS catalog name: wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat
SExtractor catalog parsing summary: zero_flux=5, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1265, passed=13307
Got 13307 stars (including 12019 good ones) from the SExtractor catalog wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat
util/solve_plate_with_UCAC5 got 13307 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 903 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 12636 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 12638 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 943 matched stars entering correct_measured_positions(), 12638 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 943 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits -region wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.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.ry02yA6if5 (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_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.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_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits
WCS_IMAGE_NAME=wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits
WCS-calibrated image found: wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits
Checking if the catalog wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits
WCS catalog name: wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=732, passed=8879
Got 8879 stars (including 8143 good ones) from the SExtractor catalog wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits.cat
util/solve_plate_with_UCAC5 got 8879 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.6'
Seting catalog search parameters based on the expected field of view 938.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013036 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010429 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 908 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.88"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 8649 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.89"
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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 8649 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.91"
Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 8649 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.99"
Excluding outliers - 935 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits -region wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.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.FDfd2JiF6m (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_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.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_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits
WCS_IMAGE_NAME=wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits
WCS-calibrated image found: wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits
Checking if the catalog wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits
WCS catalog name: wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=760, passed=8976
Got 8976 stars (including 8213 good ones) from the SExtractor catalog wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits.cat
util/solve_plate_with_UCAC5 got 8976 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.6'
Seting catalog search parameters based on the expected field of view 938.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013036 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010429 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 910 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.86"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 8715 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.90"
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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 8718 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.90"
Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 8718 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.00"
Excluding outliers - 936 stars left (next iteration limit 1029)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits -region wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.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_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits'
Saving fully-calibrated image wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits'
Saving fully-calibrated image wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits'
Saving fully-calibrated image wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits'
Preparing the HTML report for the field Aql-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20703.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20806.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20810.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20819.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20823.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20824.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20830.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20842.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20845.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20848.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20849.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20855.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20856.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20860.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20861.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20864.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20866.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20867.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20872.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20876.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20879.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20883.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20889.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20892.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20900.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20903.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20904.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20907.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out20756.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20890.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: 3s
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Considering the candidate 20756_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 20756_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
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Considering the candidate 20788_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 20788_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:44:09.68 -06:11:11.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20792_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 20792_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:53:14.22 +02:15:40.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20806_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 20806_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:46:40.02 -04:48:36.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.61, MAG_FAINT_SEARCH_LIMIT=12.59)GAIADR2_OUTPUT=# 2.781 4255141168141843456 281.66597490082 -04.81026506475 10.1486 8.6454 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.781#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20810_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 20810_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:56:17.93 +00:14:59.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.62, MAG_FAINT_SEARCH_LIMIT=12.60)GAIADR2_OUTPUT=# 2.679 4266605977677464192 284.07402200025 +00.25003798704 10.7666 9.4199 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.679#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20812_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 20812_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:39:07.55 -02:10:48.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20815_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 20815_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:37:22.40 -04:49:16.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20819_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 20819_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:34:55.55 -04:31:59.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.66, MAG_FAINT_SEARCH_LIMIT=12.64)GAIADR2_OUTPUT=# 2.716 4256851011779772800 278.73073032324 -04.53345582346 10.7447 9.4123 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.716#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20820_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 20820_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:38:08.97 -03:00:07.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20823_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 20823_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:32:23.73 -04:47:33.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.71, MAG_FAINT_SEARCH_LIMIT=12.69)GAIADR2_OUTPUT=# 2.760 4257212166958660480 278.09812971491 -04.79268997968 10.8917 9.5829 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.760#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20824_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 20824_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:43:37.74 -04:46:32.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.64, MAG_FAINT_SEARCH_LIMIT=12.62)GAIADR2_OUTPUT=# 2.469 4256655156932222208 280.90668873312 -04.77595251227 10.2604 8.6426 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.469#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20827_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 20827_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:34:11.60 -03:58:01.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20828_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 20828_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:37:20.29 -03:44:17.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20830_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 20830_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:35:53.59 -06:17:23.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.69, MAG_FAINT_SEARCH_LIMIT=12.67)GAIADR2_OUTPUT=# 1.539 4256062142203727488 278.97286268795 -06.28992126604 11.6223 11.0046 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.539#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20832_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 20832_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:43:16.94 -02:55:42.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20833_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 20833_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:43:27.36 -01:11:37.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20838_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 20838_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:27:00.14 -05:49:09.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20842_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 20842_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:32:58.58 -02:20:34.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.77, MAG_FAINT_SEARCH_LIMIT=12.75)GAIADR2_OUTPUT=# 1.256 4270167089681058560 278.24373982638 -02.34289556600 11.6836 11.0272 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.256#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20845_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 20845_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:25:34.21 -05:28:52.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.74, MAG_FAINT_SEARCH_LIMIT=12.72)GAIADR2_OUTPUT=# 4.325 4161040010868853248 276.39139020882 -05.48172081967 11.1537 9.7340 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.325#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20846_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 20846_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:29:15.80 -01:04:34.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20848_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 20848_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:33:47.40 -05:18:03.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.77, MAG_FAINT_SEARCH_LIMIT=12.75)GAIADR2_OUTPUT=# 1.642 4256430306803529472 278.44707692488 -05.30125808738 11.0061 9.7062 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.642#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20849_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 20849_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:33:12.11 -06:13:59.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.78, MAG_FAINT_SEARCH_LIMIT=12.76)GAIADR2_OUTPUT=# 1.331 4256031944312867456 278.30035592048 -06.23360553313 11.5113 10.5621 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.331#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20855_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 20855_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:29:07.55 -05:10:39.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.84, MAG_FAINT_SEARCH_LIMIT=12.82)GAIADR2_OUTPUT=# 1.715 4257095648780460544 277.28099136433 -05.17768660624 11.6609 10.8878 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.715#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20856_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 20856_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:26:55.30 -02:18:11.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.78, MAG_FAINT_SEARCH_LIMIT=12.76)GAIADR2_OUTPUT=# 1.905 4270319406402674176 276.72989003402 -02.30330712280 11.3720 10.2758 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.905#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20859_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 20859_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:39:39.62 -05:50:14.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20860_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 20860_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:30:44.05 -04:25:41.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.81, MAG_FAINT_SEARCH_LIMIT=12.79)GAIADR2_OUTPUT=# 0.851 4257301399201368576 277.68352616093 -04.42831925468 11.6688 10.9074 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.851#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20861_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 20861_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:35:51.46 -02:56:53.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.83, MAG_FAINT_SEARCH_LIMIT=12.81)GAIADR2_OUTPUT=# 0.603 4258063601275012352 278.96431064691 -02.94821301199 11.7596 11.1766 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.603#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20864_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 20864_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:25:56.96 -06:09:35.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.84, MAG_FAINT_SEARCH_LIMIT=12.82)GAIADR2_OUTPUT=# 3.026 4160921267953710080 276.48652135081 -06.15995637047 11.5627 10.5927 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.026#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20866_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 20866_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:29:14.25 -00:50:14.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.83, MAG_FAINT_SEARCH_LIMIT=12.81)GAIADR2_OUTPUT=# 0.744 4272803237528311040 277.30917409291 -00.83752121551 11.7204 10.9154 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.744#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20867_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 20867_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:33:23.19 -05:19:44.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.86, MAG_FAINT_SEARCH_LIMIT=12.84)GAIADR2_OUTPUT=# 1.733 4256407290090046080 278.34614162672 -05.32898669861 11.3514 10.1968 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.733#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20872_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 20872_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:27:24.39 -05:44:49.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 1.374 4257046789234012800 276.85127951175 -05.74733240226 11.7945 11.1610 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.374#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20874_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 20874_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:44:06.42 -03:17:20.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20876_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 20876_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:36:46.86 +02:04:23.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.84, MAG_FAINT_SEARCH_LIMIT=12.82)GAIADR2_OUTPUT=# 0.685 4279841353209941504 279.19512026104 +02.07308292879 11.8429 11.2965 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.685#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20879_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 20879_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:33:36.46 -01:11:48.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 0.871 4271992656940950656 278.40174865415 -01.19689625099 11.8383 11.2861 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.871#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20883_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 20883_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:32:28.09 +00:13:42.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.86, MAG_FAINT_SEARCH_LIMIT=12.84)GAIADR2_OUTPUT=# 0.731 4272999916968311552 278.11689407330 +00.22838847697 11.9018 11.3750 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.731#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20888_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 20888_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:37:49.49 -04:06:51.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20889_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 20889_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:25:08.15 -06:08:23.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.86, MAG_FAINT_SEARCH_LIMIT=12.84)GAIADR2_OUTPUT=# 1.323 4160935282387123328 276.28359153163 -06.13993464360 11.8866 11.2210 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.323#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20890_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 20890_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20892_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 20892_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:32:07.09 -00:20:21.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 0.512 4272942050871087232 278.02947345885 -00.33940257850 11.8773 11.3210 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.512#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20900_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 20900_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:24:33.67 -05:22:39.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.95, MAG_FAINT_SEARCH_LIMIT=12.93)GAIADR2_OUTPUT=# 3.168 4161234418276563072 276.13942847763 -05.37788385665 11.5918 10.4551 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.168#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20903_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 20903_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:24:26.72 -04:33:28.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.91, MAG_FAINT_SEARCH_LIMIT=12.89)GAIADR2_OUTPUT=# 2.001 4257433370641827840 276.11077696124 -04.55784116875 11.9715 11.4069 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20904_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 20904_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:38:39.76 -05:15:51.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.89, MAG_FAINT_SEARCH_LIMIT=12.87)GAIADR2_OUTPUT=# 0.866 4256552425654184192 279.66547668489 -05.26442623145 11.6482 10.8955 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.866#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20907_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 20907_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:28:28.05 -05:55:55.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.93, MAG_FAINT_SEARCH_LIMIT=12.91)GAIADR2_OUTPUT=# 1.518 4256277543412565760 277.11646089801 -05.93222872343 11.8324 11.2160 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.518#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11029_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 11029_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:02:20.97 +01:30:36.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20703_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 20703_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:06:03.01 -05:49:23.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.21, MAG_FAINT_SEARCH_LIMIT=12.19)GAIADR2_OUTPUT=# 1.722 4206147269239515648 286.51255906635 -05.82378368645 10.5446 9.8164 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.722#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 23s
Prepared the HTML report for the field Aql-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
18:57:37.27 -05:29:15.1
18:37:00.65 -06:14:17.2
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits
SExtractor catalog cache: saved Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat to cache
SExtractor catalog cache: saved Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
Creating symlink local_wcs_cache/wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
Creating symlink local_wcs_cache/wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits
Creating symlink local_wcs_cache/wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.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_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits exists and is non-empty
wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits exists and is non-empty
wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits exists and is non-empty
wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 18:51:25.226 -01:59:55.32
Second-epoch image center 18:51:41.246 -02:01:00.67
Angular distance between the image centers 0.0691 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 18:51:25.226 -01:59:55.32
Second-epoch image center 18:51:43.130 -02:00:55.44
Angular distance between the image centers 0.0764 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 18:51:41.246 -02:01:00.67
Second-epoch second image center 18:51:43.130 -02:00:55.44
Angular distance between the image centers 0.00798 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/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits &> /tmp/tmp.ZFVQJvM4xd
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits &> /tmp/tmp.8X6a0cssBj
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits &> /tmp/tmp.tNDOWuGkAc
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits &> /tmp/tmp.AS64d0DIhh
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits
Calibrating the magnitude scale
Found non-empty wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.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_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits and wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.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_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits and wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat
Found non-empty wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits and wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat
The reference image (wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits) and catalog (wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat) found
'wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat' -> 'wcsmag.cat'
Read 153764 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 274.9569 to 290.7986 deg, Dec -7.2966 to +3.3005 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 274.9569 to 290.7986 deg, Dec -7.2966 to 3.3005 deg
Loaded 9554 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): 6421 out of 8387 total matches.
Matched with Tycho-2 8387 out of 153764 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.669636
a=0.000000 b=1.000000 c=22.669636
From vast_summary.log: estimated ref. image limiting mag.: -7.77
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.90
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.90
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 296 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
2.1 pix Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
2.7 pix fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits
2.7 pix fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits
Limiting magnitude estimates:
14.9 mag. Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
14.9 mag. Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
14.2 mag. fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits
14.2 mag. fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits
All-image limiting magnitude estimate: 14.2 (SNR ) 13.7 (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.ZFVQJvM4xd (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits' -> 'wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
WCS_IMAGE_NAME=wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
WCS-calibrated image found: wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
Checking if the catalog wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat corresponding to the image wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits alredy exist and is non-empty...
Catalog wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat corresponding to the image wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
WCS catalog name: wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=21, blended=17867, passed=153743
Got 153743 stars (including 135593 good ones) from the SExtractor catalog wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat
util/solve_plate_with_UCAC5 got 153743 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 915 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 149678 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 149683 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 149683 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 946 stars left (next iteration limit 1040)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits -region wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.8X6a0cssBj (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits' -> 'wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
WCS_IMAGE_NAME=wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
WCS-calibrated image found: wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
Checking if the catalog wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat corresponding to the image wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits alredy exist and is non-empty...
Catalog wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat corresponding to the image wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
WCS catalog name: wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat
SExtractor catalog parsing summary: zero_flux=4, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=18180, passed=153307
Got 153307 stars (including 134827 good ones) from the SExtractor catalog wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat
util/solve_plate_with_UCAC5 got 153307 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 917 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 148895 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 148896 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 148896 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 941 stars left (next iteration limit 1035)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits -region wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.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.tNDOWuGkAc (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_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.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_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits
WCS_IMAGE_NAME=wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits
WCS-calibrated image found: wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits
Checking if the catalog wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits
WCS catalog name: wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=8845, passed=72949
Got 72949 stars (including 64028 good ones) from the SExtractor catalog wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits.cat
util/solve_plate_with_UCAC5 got 72949 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.6'
Seting catalog search parameters based on the expected field of view 938.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013036 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010429 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 933 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(), 917 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.82"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 71374 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.88"
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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 933 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(), 71373 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.88"
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 71373 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.95"
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_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits -region wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.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.AS64d0DIhh (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_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.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_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits
WCS_IMAGE_NAME=wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits
WCS-calibrated image found: wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits
Checking if the catalog wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits alredy exist and is non-empty...
Catalog wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits.cat corresponding to the image wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits
WCS catalog name: wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=8946, passed=73863
Got 73863 stars (including 64839 good ones) from the SExtractor catalog wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits.cat
util/solve_plate_with_UCAC5 got 73863 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.6'
Seting catalog search parameters based on the expected field of view 938.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013036 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010429 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 911 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.81"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 72243 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.87"
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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 72241 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.87"
Accuracy estimation diagnostic: 927 matched stars entering correct_measured_positions(), 72241 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.98"
Excluding outliers - 927 stars left (next iteration limit 1019)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits -region wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.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_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/wcs_Aql-03-Q2b1x1_2026-02-27_06-00-03_20.00sec_-14.90C_LIGHT_0051.fits
Saving fully-calibrated image wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.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_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/wcs_Aql-03-Q2b1x1_2026-02-27_06-00-40_20.00sec_-15.00C_LIGHT_0052.fits
Saving fully-calibrated image wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.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_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-09-41_20.00sec_-5.00C_LIGHT_0231.fits
Saving fully-calibrated image wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.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_2026-04-10_CI_Aql-03-Q2b1x1_040258_TTUQ2b1x1_19498_xDnQlVcJ/wcs_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232.fits
Preparing the HTML report for the field Aql-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out101137.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out126504.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out164546.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out164660.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out164747.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out165098.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out169875.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out171873.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177233.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177234.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177238.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177239.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177244.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177250.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177255.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177256.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177261.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177269.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177276.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177295.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177296.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177299.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177300.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177312.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177314.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177331.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177333.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177339.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177341.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177347.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177350.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177353.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177360.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177367.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177371.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177499.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177570.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177629.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177645.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177657.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177676.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177686.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177708.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177718.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177724.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177729.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177749.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177750.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177758.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177764.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177767.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177776.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177777.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177795.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177796.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177802.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177805.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177806.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177812.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177841.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177850.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177864.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177871.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177889.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177892.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177920.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177927.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177932.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out177946.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out26244.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out27317.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out36147.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out39780.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out43917.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out46957.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out65751.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75100.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out95944.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out101791.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out117236.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out121802.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out122243.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out123468.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out125106.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out125264.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out129218.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out129625.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131191.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131964.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133804.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134604.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136619.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151421.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out152718.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out164443.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out164908.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out164952.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out167514.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out169659.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177246.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177260.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177264.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177301.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177307.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177310.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177343.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177354.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177355.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177772.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177798.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out177894.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22662.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22724.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25664.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29210.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31423.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31932.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out32981.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out34774.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36284.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36470.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out36671.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37930.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out38488.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39096.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out39715.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out41593.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43918.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45015.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out46882.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out48037.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53184.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55734.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55987.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56873.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out58254.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out59471.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out60047.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out60822.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out62374.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out63556.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out64430.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65965.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66056.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67549.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out68026.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out71054.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75011.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out76012.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out76302.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out80585.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out81025.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82275.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out83538.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out86723.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out89426.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out90097.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out91786.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out92194.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out96643.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 58s
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: 46s
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Considering the candidate 177233_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177233_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:08:04.44 -06:06:33.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 2.662 4205934238862235904 287.01891963447 -06.10875049926 12.4979 11.7906 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.662#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177234_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177234_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:02:30.70 -01:36:44.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)
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Considering the candidate 177238_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177238_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:01:43.91 +00:45:31.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)
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Considering the candidate 177239_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177239_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:57:01.50 -00:49:34.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)
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Considering the candidate 177244_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177244_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:06:50.81 +00:22:58.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 2.827 4267185763908784000 286.71097464702 +00.38330774860 13.0594 11.7756 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.827#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177246_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 177246_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
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Considering the candidate 177250_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177250_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:37:22.67 -03:11:05.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)
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Considering the candidate 177255_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177255_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:01:12.53 +00:07:30.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)
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Considering the candidate 177256_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177256_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:00:31.43 -02:58:50.3 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 177260_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 177260_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
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Considering the candidate 177261_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177261_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:06:20.61 +01:38:01.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)
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Considering the candidate 177264_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 177264_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
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Considering the candidate 177269_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177269_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:57:10.92 -05:53:36.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)
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Considering the candidate 177275_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177275_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 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 177276_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177276_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:05:22.11 -05:22:17.0 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 177295_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177295_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:56:21.61 -04:22:38.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 3.471 4255366877256163200 284.09029492351 -04.37637505772 13.4070 12.5846 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.471#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177296_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177296_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:07:30.94 -02:08:55.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 1.491 4262102343698036352 286.87852244328 -02.14873855466 12.8199 11.7991 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.491#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177297_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177297_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 177299_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177299_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:06:53.20 -05:08:43.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)
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Considering the candidate 177300_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177300_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:38:29.85 -02:10:25.7 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 177301_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 177301_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
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Considering the candidate 177307_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 177307_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
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Considering the candidate 177308_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177308_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 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 177310_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 177310_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
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Considering the candidate 177311_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177311_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:05:47.95 -00:18:47.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177312_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177312_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:56:57.17 -04:48:27.6 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 177313_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177313_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:07:14.68 -06:04:08.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177314_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177314_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:39:27.34 -02:58:20.2 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 177331_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177331_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:08:22.51 -01:18:51.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)
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Considering the candidate 177333_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177333_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:09:07.21 +01:51:59.5 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 177334_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177334_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 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 177338_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177338_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:55:58.38 -02:11:04.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177339_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177339_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:53:31.45 -05:39:07.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)
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Considering the candidate 177341_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177341_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:04:23.09 -00:16:00.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)
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Considering the candidate 177343_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 177343_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
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Considering the candidate 177345_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177345_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:08:29.83 -01:55:18.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177347_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177347_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:55:54.06 -05:49:47.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)
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Considering the candidate 177350_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177350_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:09:06.88 +01:34:40.1 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 177353_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177353_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:03:07.02 -05:16:15.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 1.297 4254275985569178240 285.77889135836 -05.27113063125 12.0632 10.6009 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.297#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177354_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 177354_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
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Considering the candidate 177355_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 177355_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
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Considering the candidate 177360_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177360_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:55:10.56 -05:31:30.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.42, MAG_FAINT_SEARCH_LIMIT=13.40)
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Considering the candidate 177363_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177363_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:08:15.46 -04:11:54.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177365_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177365_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:03:31.70 -05:44:28.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177367_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177367_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:05:43.56 -00:17:00.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 1.044 4265625247685090560 286.43126285515 -00.28322173289 12.1938 11.1508 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.044#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177371_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177371_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:08:10.58 -05:34:32.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.74, MAG_FAINT_SEARCH_LIMIT=12.72)GAIADR2_OUTPUT=# 2.237 4206238464309828992 287.04450415184 -05.57601464750 11.2753 10.0060 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.237#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177413_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177413_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:47:01.87 -04:44:30.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177422_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177422_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:02:58.70 -03:43:12.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 177474_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177474_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:07:37.21 +00:06:07.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177478_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177478_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:05:13.42 +01:52:39.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177481_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177481_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:07:43.86 -02:25:22.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177482_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177482_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:57:32.11 -06:14:41.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177499_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177499_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:55:03.71 -03:39:07.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)GAIADR2_OUTPUT=# 1.237 4255662710251617536 283.76532728803 -03.65162674691 10.8115 9.4133 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.237#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177506_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177506_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:56:59.94 -05:52:58.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177518_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177518_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:04:34.32 -05:39:45.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177521_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177521_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:05:31.55 -00:39:18.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177570_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177570_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:07:00.01 +00:45:12.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 2.146 4267272109932407808 286.75009093798 +00.75403858480 12.3422 10.9153 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.146#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177579_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177579_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:08:04.12 -03:51:00.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177580_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177580_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:07:51.35 -05:52:35.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177582_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177582_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:24:32.36 -01:32:06.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177586_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177586_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:53:10.82 -04:45:06.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177587_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177587_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:33:17.37 -05:55:01.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 177607_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177607_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:57:51.15 -01:59:01.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177623_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177623_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:48:28.66 -05:40:49.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177628_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177628_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:24:32.42 -03:31:23.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177629_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177629_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:59:30.47 -05:14:41.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 3.256 4254497296638897408 284.87727259706 -05.24562624756 12.9173 10.8211 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.256#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177632_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177632_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:07:29.06 -01:36:09.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177634_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177634_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:05:21.19 -03:18:35.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177638_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177638_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:08:01.12 -05:10:59.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177645_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177645_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:27:26.73 +01:30:12.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 1.326 4276754989701351936 276.86124403017 +01.50298905465 13.5542 12.6214 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.326#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177646_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177646_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:27:14.93 +00:53:34.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177657_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177657_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:43:16.51 -01:37:40.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 3.927 4259945140547634176 280.81842456444 -01.62686149381 12.7908 11.5175 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.927#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177659_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177659_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:59:12.18 +00:14:15.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177661_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177661_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:04:49.03 -01:12:46.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177665_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177665_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:52:05.13 -05:12:18.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177672_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177672_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:54:59.22 -01:02:09.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177676_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177676_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:54:22.52 -01:03:15.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 1.389 4265257529756500992 283.59346573308 -01.05410480784 13.0338 11.8814 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.389#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177683_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177683_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:07:42.91 +00:35:08.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177686_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177686_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:40:03.33 -05:31:45.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 5.574 4256493911015051008 280.01263854591 -05.53016195730 11.4427 9.7849 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.574#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177692_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177692_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:01:27.31 -01:49:48.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177695_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177695_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:52:10.75 -06:00:02.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177697_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177697_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:26:53.93 -05:26:58.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177699_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177699_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:06:26.63 -04:13:54.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177704_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177704_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:01:10.54 -05:38:58.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177708_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177708_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:04:46.08 -05:10:21.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 4.456 4254360579240770944 286.19261573332 -05.17374173838 12.3744 10.8026 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.456#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177709_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177709_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:53:19.31 -05:02:40.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177713_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177713_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:08:47.65 +01:51:13.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177715_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177715_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:05:04.58 +01:15:59.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177718_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177718_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:02:14.09 -05:56:33.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 3.936 4206174791394602752 285.55912868393 -05.94367684285 12.5495 11.1178 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.936#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177724_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177724_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:09:11.36 -05:11:40.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 4.494 4206287044655531008 287.29834250894 -05.19524047102 11.9769 10.3337 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.494#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177726_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177726_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:08:20.78 -05:53:37.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177729_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177729_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:38:37.95 -03:05:46.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 3.619 4259358821667952640 279.65727284254 -03.09557574246 12.4869 10.9360 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.619#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177744_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177744_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:03:57.16 -06:11:50.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177749_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177749_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:57:47.15 +00:04:48.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 2.040 4265850892411484288 284.44682436206 +00.08054377625 11.7163 9.9759 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.040#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177750_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177750_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:54:53.65 -00:42:47.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 2.632 4265408231568446976 283.72353506797 -00.71235218682 11.9843 10.3161 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.632#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177758_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177758_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:33:44.02 -06:01:27.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 4.067 4256041938681598464 278.43265878397 -06.02500836860 12.3400 10.3151 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.067#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177764_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177764_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:59:02.72 -05:30:25.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 1.860 4253929197091897344 284.76157453379 -05.50765181297 12.4333 10.9079 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.860#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177767_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177767_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:42:15.81 +00:08:04.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 3.950 4272477064839677568 280.56539454320 +00.13365243318 13.8538 13.0050 NOT_AVAILABLE#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 177772_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 177772_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
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Considering the candidate 177776_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177776_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:44:47.84 -04:45:35.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 0.883 4256652545589437312 281.19911282777 -04.75999780628 11.8660 10.3320 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.883#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 177777_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177777_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:01:55.69 -04:22:28.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 3.263 4254663254177299328 285.48283626595 -04.37493997934 12.4959 10.9659 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.263#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177778_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177778_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:09:15.03 -02:38:34.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177787_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177787_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:08:54.62 +01:38:28.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177795_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177795_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:03:27.49 -02:12:48.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 0.382 4261772460191067776 285.86460156696 -02.21367101979 12.6704 11.2418 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.382#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177796_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177796_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:24:36.19 -00:01:08.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)GAIADR2_OUTPUT=# 3.108 4273152920894278016 276.14992871839 -00.01897695666 13.0799 11.5302 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.108#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177798_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 177798_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
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Considering the candidate 177802_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177802_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:36:46.96 -01:53:25.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.75, MAG_FAINT_SEARCH_LIMIT=14.73)GAIADR2_OUTPUT=# 3.858 4259699945144471936 279.19462317063 -01.89055207025 11.9150 10.2517 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.858#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177805_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177805_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:54:28.27 -03:23:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 4.404 4255688106435735936 283.61741665116 -03.40013695058 13.5606 11.3860 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.404#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177806_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177806_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:44:09.09 -00:05:37.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 2.756 4272413048341314432 281.03711227053 -00.09362926427 12.0521 10.4238 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.756#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177812_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177812_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:42:09.97 -01:07:26.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)GAIADR2_OUTPUT=# 0.325 4260229845357070336 280.54146956350 -01.12416542700 12.4654 10.9067 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.325#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177823_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177823_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:53:41.08 -05:03:55.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177826_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177826_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:59:55.56 -03:17:55.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177841_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177841_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:55:59.11 -04:02:33.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)
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Considering the candidate 177847_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177847_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:06:55.15 -01:31:20.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177850_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177850_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:09:12.12 -00:44:32.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 4.078 4262554964528000512 287.30142506562 -00.74179056577 12.4312 10.7301 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.078#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177864_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177864_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:49:58.39 -00:56:48.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 0.777 4266054027183943296 282.49342532153 -00.94705832755 13.1773 11.7663 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.777#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177871_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177871_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:59:56.37 -05:30:14.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 2.572 4254289179704633856 284.98524610943 -05.50450052136 12.8806 11.4500 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.572#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177878_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177878_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:06:57.47 -04:56:10.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177882_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177882_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:03:12.70 -00:47:45.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177889_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177889_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:07:58.79 -04:23:26.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 5.112 4260422221206272384 286.99531985901 -04.39217898598 12.5783 10.8592 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.112#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177892_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177892_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:50:44.62 -03:46:18.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 1.014 4255331727230735488 282.68596741087 -03.77208265767 12.8670 11.4038 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.014#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177894_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 177894_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
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Considering the candidate 177920_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177920_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:35:44.71 +01:06:38.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)GAIADR2_OUTPUT=# 1.515 4273574239993367808 278.93605695242 +01.11045617630 13.6381 12.2937 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.515#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177927_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177927_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:48:26.60 -00:14:37.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)GAIADR2_OUTPUT=# 3.915 4266332096203471104 282.10974596745 -00.24382348307 12.7831 11.2145 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.915#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177932_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177932_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:53:25.47 -02:52:21.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.08, MAG_FAINT_SEARCH_LIMIT=15.06)GAIADR2_OUTPUT=# 1.786 4258859093625712896 283.35637775903 -02.87306585871 12.7071 11.2129 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.786#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 177946_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177946_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:53:54.47 -00:20:21.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)
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Considering the candidate 177947_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 177947_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:56:13.30 -02:24:54.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52238_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 52238_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:05:03.76 -04:45:02.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 132154_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 132154_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:44:18.96 -00:00:13.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 76012_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 76012_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
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Considering the candidate 25904_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 25904_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:05:29.53 -06:04:54.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 41503_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 41503_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:56:04.62 -05:21:53.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 146622_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 146622_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:09:09.18 +01:17:24.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56749_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 56749_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:49:15.65 -04:29:18.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25664_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 25664_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
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Considering the candidate 138147_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 138147_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:56:08.71 -00:28:34.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 129625_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 129625_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
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Considering the candidate 27946_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 27946_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:56:17.17 -06:01:21.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 142751_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 142751_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:00:59.65 -00:48:43.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 115835_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 115835_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:53:57.46 +01:36:35.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 136619_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 136619_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 95944_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 95944_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:49:24.67 -01:29:03.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 1.827 4259267669587338880 282.35251519112 -01.48388005473 11.3173 9.7442 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.827#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 39045_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 39045_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:33:07.32 -05:30:10.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 129218_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 129218_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 60822_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 60822_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
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Considering the candidate 66890_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 66890_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:49:23.30 -03:46:37.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 81025_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 81025_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
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Considering the candidate 98233_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 98233_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:59:11.47 -01:19:13.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 152718_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 152718_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
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Considering the candidate 32562_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 32562_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:56:55.36 -05:48:54.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 146876_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 146876_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:02:20.96 +01:30:36.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 139652_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 139652_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:54:34.94 -00:35:06.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 96276_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 96276_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:42:11.80 -01:28:22.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 91786_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 91786_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
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Considering the candidate 87924_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 87924_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:01:58.44 -02:00:47.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29210_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 29210_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
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Considering the candidate 65751_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 65751_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:50:43.99 -03:51:26.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.25, MAG_FAINT_SEARCH_LIMIT=14.23)GAIADR2_OUTPUT=# 2.785 4255330043603416448 282.68397537846 -03.85769818192 11.7833 10.1914 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.785#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 60047_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 60047_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125264_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 125264_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
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Considering the candidate 68026_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 68026_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
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Considering the candidate 169659_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 169659_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 117236_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 117236_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 75227_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 75227_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:08:59.21 -03:01:46.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 49595_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 49595_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:37:12.99 -04:57:06.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 65965_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 65965_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 122243_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 122243_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 75955_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 75955_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:58:15.53 -03:00:01.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 139263_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 139263_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:59:29.71 -00:34:24.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 147796_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 147796_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:02:39.94 +02:11:51.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 82275_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 82275_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 83700_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 83700_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:01:40.77 -02:21:00.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62374_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 62374_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 50838_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 50838_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:39:48.45 -04:52:45.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103890_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 103890_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:51:53.77 -00:58:46.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22456_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 22456_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:47:21.50 -06:16:12.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 142804_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 142804_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:05:52.13 -00:49:03.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 57707_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 57707_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:02:39.31 -04:19:10.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 74720_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 74720_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:04:01.03 -03:05:10.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 73075_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 73075_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:52:35.94 -03:12:15.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125106_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 125106_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 48037_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 48037_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 138427_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 138427_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:24:51.08 -00:32:32.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22662_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 22662_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31780_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 31780_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:02:52.85 -05:50:28.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 70335_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 70335_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:43:24.43 -03:30:11.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131191_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 131191_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70668_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 70668_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:06:12.80 -03:24:37.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 45130_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 45130_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:04:04.70 -05:09:18.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 92194_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 92194_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 165533_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 165533_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:56:26.43 -00:58:36.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 134604_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 134604_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 165098_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 165098_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:09:11.94 -02:21:09.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 5.278 4261335193811439744 287.30116133341 -02.35301213044 12.2234 11.2886 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.278#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39096_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 39096_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29776_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 29776_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:07:27.79 -05:54:15.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 165079_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 165079_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:08:07.16 -01:34:51.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 38488_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 38488_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 165073_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 165073_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:09:00.96 +00:21:09.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 80585_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 80585_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 164952_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 164952_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 86723_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 86723_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 164908_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 164908_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 164747_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 164747_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:06:15.32 +01:11:39.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 85292_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 85292_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:01:40.35 -02:11:58.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36671_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 36671_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 95332_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 95332_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:06:05.51 -01:29:59.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 164660_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 164660_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:00:19.06 -05:37:18.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.17, MAG_FAINT_SEARCH_LIMIT=14.15)GAIADR2_OUTPUT=# 5.361 4254284304965411072 285.08047491697 -05.62274747082 12.4731 11.1113 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.361#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 75100_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 75100_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:50:17.86 -03:05:30.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 4.460 4258749249845413504 282.57327701694 -03.09218422115 11.6686 9.9298 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.460#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 164556_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 164556_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:07:40.04 -05:07:20.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 164546_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 164546_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:36:25.22 -03:23:55.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 43918_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 43918_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 73022_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 73022_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:59:53.77 -03:14:29.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 99382_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 99382_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:06:05.36 -01:12:16.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 73869_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 73869_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:01:04.89 -03:10:47.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 66056_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 66056_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39715_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 39715_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 164443_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 164443_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 142326_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 142326_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:58:34.43 -00:47:36.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 59471_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 59471_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 146304_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 146304_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:53:14.21 +02:15:39.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 68736_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 68736_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:05:24.23 -03:35:46.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32981_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 32981_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131964_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 131964_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71757_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 71757_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:04:05.08 -03:20:38.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35000_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 35000_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:06:36.87 -05:39:46.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 169875_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 169875_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:00:38.74 -02:13:32.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 1.865 4261877905890320256 285.16193507017 -02.22575389429 11.7223 10.1665 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.865#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 58254_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 58254_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 67549_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 67549_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103039_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 103039_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:52:48.43 -01:01:23.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 84634_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 84634_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:58:42.89 -02:16:38.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 121802_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 121802_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53184_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 53184_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46957_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 46957_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:32:24.10 -05:05:51.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23823_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 23823_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:54:04.85 -06:12:23.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 126971_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 126971_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:02:56.67 +00:25:46.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 73000_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 73000_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:43:44.88 -03:16:11.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35089_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 35089_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:43:01.55 -05:42:32.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26244_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 26244_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:55:21.45 -06:05:46.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 3.446 4253969771583459200 283.84001252793 -06.09696730371 12.1900 10.6862 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.446#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 83538_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 83538_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131573_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 131573_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:04:28.00 +00:03:05.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 92087_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 92087_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:58:01.64 -01:43:52.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55734_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 55734_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33038_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 33038_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:55:16.83 -05:47:49.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 85109_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 85109_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:08:58.37 -02:13:45.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 64430_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 64430_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26928_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 26928_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:49:54.88 -06:04:32.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 83983_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 83983_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:42:23.71 -02:22:02.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133804_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 133804_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22724_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 22724_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27317_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 27317_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:37:37.65 -06:03:55.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 5.205 4256084132438009856 279.40571942440 -06.06626623434 11.6634 10.1102 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.205#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46882_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 46882_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 71054_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 71054_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56873_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 56873_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55987_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 55987_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34774_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 34774_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37930_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 37930_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 173105_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 173105_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:03:24.58 -00:32:37.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31238_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 31238_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:34:21.24 -05:53:17.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36470_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 36470_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 94085_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 94085_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:07:08.68 -01:34:27.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41887_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 41887_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:07:40.02 -05:19:37.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31932_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 31932_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 60096_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 60096_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:42:32.02 -04:17:10.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 75011_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 75011_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 45015_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 45015_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 43917_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 43917_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:07:50.20 -05:13:28.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 5.402 4206330720210959104 286.96017241718 -05.22570074677 12.2786 11.3267 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.402#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 83576_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 83576_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:08:00.30 -02:19:19.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 63556_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 63556_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101137_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 101137_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:02:33.44 -01:07:20.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 2.887 4262471401641458944 285.64001928269 -01.12194521318 11.2906 9.7583 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.887#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 123468_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 123468_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51284_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 51284_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:24:41.56 -04:51:19.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 90097_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 90097_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167525_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 167525_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:41:07.33 -01:35:10.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 167514_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 167514_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31955_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 31955_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:09:12.27 -05:48:46.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31962_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 31962_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:08:37.13 -05:48:07.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 84001_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 84001_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:58:41.82 -02:20:12.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 28067_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 28067_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:07:38.71 -05:58:53.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36147_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 36147_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:45:29.86 -05:39:32.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22207_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 22207_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:45:34.45 -06:17:17.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 46681_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 46681_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:06:55.03 -05:03:22.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39602_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 39602_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:48:41.22 -05:27:55.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 26510_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 26510_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:07:48.09 -06:03:05.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 89426_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 89426_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 84941_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 84941_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 19:09:06.56 -02:14:03.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 39780_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 39780_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:41:21.07 -05:29:03.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22997_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 22997_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:31:13.04 -06:14:39.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 151421_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 151421_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23552_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 23552_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:43:36.08 -06:14:01.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31423_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 31423_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 101791_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 101791_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 36284_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 36284_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 41593_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 41593_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 76302_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 76302_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 126504_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 126504_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:56:30.05 +00:30:31.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 2.200 4266631373832058368 284.12548463740 +00.50915617529 11.1810 9.5624 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.200#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 96643_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
Preparing report for the candidate 96643_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 171873_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232
The candidate 171873_fd_Aql-03-Q2b1x1_2026-04-10_03-10-29_20.00sec_-4.90C_LIGHT_0232 did not pass the final checks
**** FOUND 18:37:39.34 -03:53:02.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 2.506 4257743128019956096 279.41328229622 -03.88426223312 11.8490 10.1960 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.506#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 5s
make_report_in_HTML.sh TOTAL: 109s
Prepared the HTML report for the field Aql-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
18:57:37.27 -05:29:15.1
18:37:00.65 -06:14:17.2
18:53:20.09 -01:06:45.8
18:57:51.49 +01:23:37.2
19:09:17.50 +00:53:31.1
19:07:10.27 +00:51:33.2
18:30:06.26 +00:42:33.2
19:02:41.46 +00:36:11.0
18:56:34.08 +00:35:13.9
18:54:02.33 +00:15:32.1
19:01:40.93 +00:14:12.9
19:07:55.14 +00:05:32.5
18:55:40.63 +00:01:18.9
19:09:00.29 -00:08:19.6
19:05:07.90 -00:11:37.1
19:02:14.17 -00:19:09.7
19:06:48.21 +01:30:09.4
18:53:28.75 +01:21:53.6
18:48:44.83 -05:05:53.0
19:08:26.41 +00:26:14.5
18:51:17.90 -05:02:57.4
18:58:09.94 -03:26:39.8
18:51:44.49 -05:55:51.3
18:59:50.33 -01:35:05.2
18:52:46.46 -01:21:21.8
19:07:10.67 -01:04:48.3
19:00:56.42 -04:12:05.4
19:05:15.57 +01:54:04.9
19:06:28.28 -02:44:10.0
19:08:29.90 -00:27:24.4
19:03:46.28 -05:55:58.8
18:46:17.00 -06:13:37.1
18:24:06.80 +01:54:53.7
18:49:52.01 -05:42:04.5
19:08:24.24 +01:57:43.2
19:01:35.40 -06:13:59.6
19:08:13.12 -06:12:42.6
18:40:10.38 -06:08:15.7
18:29:55.91 -05:58:20.4
18:26:58.99 -05:52:13.3
19:06:02.99 -05:49:23.1
18:56:27.63 -05:47:52.3
18:40:13.59 -05:43:15.2
18:50:04.54 -05:38:36.8
18:47:40.78 -05:38:14.9
19:08:12.20 -05:34:52.8
19:07:01.34 -05:31:54.9
19:07:31.27 -05:29:33.6
19:08:10.86 -05:28:04.5
18:45:51.57 -05:28:45.4
18:54:17.87 -05:22:28.8
19:06:40.91 -05:13:22.7
18:43:25.96 -05:11:44.3
18:50:25.00 -05:06:05.7
18:50:46.75 -05:02:07.4
19:08:24.09 -04:41:30.1
19:06:11.74 -04:31:52.6
18:52:22.14 -04:33:22.1
19:09:24.45 -04:26:51.3
18:54:30.37 -04:23:53.2
19:07:28.90 -04:16:28.7
18:46:58.12 -04:16:24.9
18:47:27.02 -04:13:13.8
18:52:56.32 -04:06:44.0
19:05:23.30 -03:59:43.1
19:03:12.03 -03:55:58.3
19:00:02.75 -03:49:07.0
18:58:03.41 -03:49:01.3
19:03:53.59 -03:41:36.2
18:36:24.26 -03:41:32.2
18:51:37.37 -03:26:10.5
19:08:39.31 -03:02:06.6
18:46:32.18 -02:57:20.9
18:52:24.28 -02:59:00.1
19:06:55.01 -02:33:46.1
18:27:38.03 -02:35:57.1
18:55:32.50 -02:28:48.5
19:00:20.12 -02:22:05.7
19:09:21.00 -02:07:30.6
18:56:20.56 -01:56:14.9
19:05:49.50 -01:51:55.8
18:55:48.92 -01:45:58.0
19:05:19.23 -01:42:24.8
18:56:56.21 -01:25:38.8
########### Completed Aql-03-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
18:57:37.27 -05:29:15.1
18:37:00.65 -06:14:17.2
18:59:50.33 -01:35:05.2
18:52:46.46 -01:21:21.8
19:07:10.67 -01:04:48.3
19:00:56.42 -04:12:05.4
19:05:15.57 +01:54:04.9
19:06:28.28 -02:44:10.0
19:08:29.90 -00:27:24.4
19:03:46.28 -05:55:58.8
18:46:17.00 -06:13:37.1
18:24:06.80 +01:54:53.7
18:49:52.01 -05:42:04.5
19:08:24.24 +01:57:43.2
18:46:32.18 -02:57:20.9
18:40:10.38 -06:08:15.7
19:01:40.93 +00:14:12.9
19:02:14.17 -00:19:09.7
18:54:02.33 +00:15:32.1
18:47:27.02 -04:13:13.8
18:27:38.03 -02:35:57.1
18:53:28.75 +01:21:53.6
18:55:48.92 -01:45:58.0
18:29:55.91 -05:58:20.4
18:46:58.12 -04:16:24.9
18:56:34.08 +00:35:13.9
18:36:24.26 -03:41:32.2
18:51:44.49 -05:55:51.3
18:57:51.49 +01:23:37.2
19:00:02.75 -03:49:07.0
19:07:10.27 +00:51:33.2
18:55:32.50 -02:28:48.5
18:52:56.32 -04:06:44.0
19:02:41.46 +00:36:11.0
18:50:46.75 -05:02:07.4
19:01:35.40 -06:13:59.6
19:07:55.14 +00:05:32.5
19:05:19.23 -01:42:24.8
19:05:07.90 -00:11:37.1
19:08:10.86 -05:28:04.5
19:07:31.27 -05:29:33.6
19:06:55.01 -02:33:46.1
18:51:17.90 -05:02:57.4
19:09:21.00 -02:07:30.6
19:08:26.41 +00:26:14.5
19:08:12.20 -05:34:52.8
19:06:40.91 -05:13:22.7
18:58:03.41 -03:49:01.3
18:45:51.57 -05:28:45.4
18:48:44.83 -05:05:53.0
19:07:28.90 -04:16:28.7
18:56:27.63 -05:47:52.3
18:55:40.63 +00:01:18.9
18:54:30.37 -04:23:53.2
19:03:53.59 -03:41:36.2
19:09:17.50 +00:53:31.1
19:08:24.09 -04:41:30.1
19:00:20.12 -02:22:05.7
19:06:11.74 -04:31:52.6
19:03:12.03 -03:55:58.3
19:09:00.29 -00:08:19.6
19:08:13.12 -06:12:42.6
18:50:25.00 -05:06:05.7
18:51:37.37 -03:26:10.5
19:09:24.45 -04:26:51.3
18:52:22.14 -04:33:22.1
18:40:13.59 -05:43:15.2
19:07:01.34 -05:31:54.9
18:47:40.78 -05:38:14.9
19:06:02.99 -05:49:23.1
19:08:39.31 -03:02:06.6
18:43:25.96 -05:11:44.3
19:05:23.30 -03:59:43.1
18:30:06.26 +00:42:33.2
19:05:49.50 -01:51:55.8
18:58:09.94 -03:26:39.8
18:56:20.56 -01:56:14.9
19:06:48.21 +01:30:09.4
18:26:58.99 -05:52:13.3
18:53:20.09 -01:06:45.8
18:50:04.54 -05:38:36.8
18:54:17.87 -05:22:28.8
18:52:24.28 -02:59:00.1
18:56:56.21 -01:25:38.8
###################################################################################
18:57:37.27 -05:29:15.1 -- not an asteroid (will add it to exclusion list)
18:37:00.65 -06:14:17.2 -- not an asteroid (will add it to exclusion list)
18:59:50.33 -01:35:05.2 -- not an asteroid (will add it to exclusion list)
18:52:46.46 -01:21:21.8 -- not an asteroid (will add it to exclusion list)
19:07:10.67 -01:04:48.3 -- not an asteroid (will add it to exclusion list)
19:00:56.42 -04:12:05.4 -- not an asteroid (will add it to exclusion list)
19:05:15.57 +01:54:04.9 -- not an asteroid (will add it to exclusion list)
19:06:28.28 -02:44:10.0 -- not an asteroid (will add it to exclusion list)
19:08:29.90 -00:27:24.4 -- not an asteroid (will add it to exclusion list)
19:03:46.28 -05:55:58.8 -- not an asteroid (will add it to exclusion list)
18:46:17.00 -06:13:37.1 -- not an asteroid (will add it to exclusion list)
18:24:06.80 +01:54:53.7 -- not an asteroid (will add it to exclusion list)
18:49:52.01 -05:42:04.5 -- not an asteroid (will add it to exclusion list)
19:08:24.24 +01:57:43.2 -- not an asteroid (will add it to exclusion list)
18:46:32.18 -02:57:20.9 -- not an asteroid (will add it to exclusion list)
18:40:10.38 -06:08:15.7 -- not an asteroid (will add it to exclusion list)
19:01:40.93 +00:14:12.9 -- not an asteroid (will add it to exclusion list)
19:02:14.17 -00:19:09.7 -- not an asteroid (will add it to exclusion list)
18:54:02.33 +00:15:32.1 -- not an asteroid (will add it to exclusion list)
18:47:27.02 -04:13:13.8 -- not an asteroid (will add it to exclusion list)
18:27:38.03 -02:35:57.1 -- not an asteroid (will add it to exclusion list)
18:53:28.75 +01:21:53.6 -- not an asteroid (will add it to exclusion list)
18:55:48.92 -01:45:58.0 -- not an asteroid (will add it to exclusion list)
18:29:55.91 -05:58:20.4 -- not an asteroid (will add it to exclusion list)
18:46:58.12 -04:16:24.9 -- not an asteroid (will add it to exclusion list)
18:56:34.08 +00:35:13.9 -- not an asteroid (will add it to exclusion list)
18:36:24.26 -03:41:32.2 -- not an asteroid (will add it to exclusion list)
18:51:44.49 -05:55:51.3 -- not an asteroid (will add it to exclusion list)
18:57:51.49 +01:23:37.2 -- not an asteroid (will add it to exclusion list)
19:00:02.75 -03:49:07.0 -- not an asteroid (will add it to exclusion list)
19:07:10.27 +00:51:33.2 -- not an asteroid (will add it to exclusion list)
18:55:32.50 -02:28:48.5 -- not an asteroid (will add it to exclusion list)
18:52:56.32 -04:06:44.0 -- not an asteroid (will add it to exclusion list)
19:02:41.46 +00:36:11.0 -- not an asteroid (will add it to exclusion list)
18:50:46.75 -05:02:07.4 -- not an asteroid (will add it to exclusion list)
19:01:35.40 -06:13:59.6 -- not an asteroid (will add it to exclusion list)
19:07:55.14 +00:05:32.5 -- not an asteroid (will add it to exclusion list)
19:05:19.23 -01:42:24.8 -- not an asteroid (will add it to exclusion list)
19:05:07.90 -00:11:37.1 -- not an asteroid (will add it to exclusion list)
19:08:10.86 -05:28:04.5 -- not an asteroid (will add it to exclusion list)
19:07:31.27 -05:29:33.6 -- not an asteroid (will add it to exclusion list)
19:06:55.01 -02:33:46.1 -- not an asteroid (will add it to exclusion list)
18:51:17.90 -05:02:57.4 -- not an asteroid (will add it to exclusion list)
19:09:21.00 -02:07:30.6 -- not an asteroid (will add it to exclusion list)
19:08:26.41 +00:26:14.5 -- not an asteroid (will add it to exclusion list)
19:08:12.20 -05:34:52.8 -- not an asteroid (will add it to exclusion list)
19:06:40.91 -05:13:22.7 -- not an asteroid (will add it to exclusion list)
18:58:03.41 -03:49:01.3 -- not an asteroid (will add it to exclusion list)
18:45:51.57 -05:28:45.4 -- not an asteroid (will add it to exclusion list)
18:48:44.83 -05:05:53.0 -- not an asteroid (will add it to exclusion list)
19:07:28.90 -04:16:28.7 -- not an asteroid (will add it to exclusion list)
18:56:27.63 -05:47:52.3 -- not an asteroid (will add it to exclusion list)
18:55:40.63 +00:01:18.9 -- not an asteroid (will add it to exclusion list)
18:54:30.37 -04:23:53.2 -- not an asteroid (will add it to exclusion list)
19:03:53.59 -03:41:36.2 -- not an asteroid (will add it to exclusion list)
19:09:17.50 +00:53:31.1 -- not an asteroid (will add it to exclusion list)
19:08:24.09 -04:41:30.1 -- not an asteroid (will add it to exclusion list)
19:00:20.12 -02:22:05.7 -- not an asteroid (will add it to exclusion list)
19:06:11.74 -04:31:52.6 -- not an asteroid (will add it to exclusion list)
19:03:12.03 -03:55:58.3 -- not an asteroid (will add it to exclusion list)
19:09:00.29 -00:08:19.6 -- not an asteroid (will add it to exclusion list)
19:08:13.12 -06:12:42.6 -- not an asteroid (will add it to exclusion list)
18:50:25.00 -05:06:05.7 -- not an asteroid (will add it to exclusion list)
18:51:37.37 -03:26:10.5 -- not an asteroid (will add it to exclusion list)
19:09:24.45 -04:26:51.3 -- not an asteroid (will add it to exclusion list)
18:52:22.14 -04:33:22.1 -- not an asteroid (will add it to exclusion list)
18:40:13.59 -05:43:15.2 -- not an asteroid (will add it to exclusion list)
19:07:01.34 -05:31:54.9 -- not an asteroid (will add it to exclusion list)
18:47:40.78 -05:38:14.9 -- not an asteroid (will add it to exclusion list)
19:06:02.99 -05:49:23.1 -- not an asteroid (will add it to exclusion list)
19:08:39.31 -03:02:06.6 -- not an asteroid (will add it to exclusion list)
18:43:25.96 -05:11:44.3 -- not an asteroid (will add it to exclusion list)
19:05:23.30 -03:59:43.1 -- not an asteroid (will add it to exclusion list)
18:30:06.26 +00:42:33.2 -- not an asteroid (will add it to exclusion list)
19:05:49.50 -01:51:55.8 -- not an asteroid (will add it to exclusion list)
18:58:09.94 -03:26:39.8 -- not an asteroid (will add it to exclusion list)
18:56:20.56 -01:56:14.9 -- not an asteroid (will add it to exclusion list)
19:06:48.21 +01:30:09.4 -- not an asteroid (will add it to exclusion list)
18:26:58.99 -05:52:13.3 -- not an asteroid (will add it to exclusion list)
18:53:20.09 -01:06:45.8 -- not an asteroid (will add it to exclusion list)
18:50:04.54 -05:38:36.8 -- not an asteroid (will add it to exclusion list)
18:54:17.87 -05:22:28.8 -- not an asteroid (will add it to exclusion list)
18:52:24.28 -02:59:00.1 -- not an asteroid (will add it to exclusion list)
18:56:56.21 -01:25:38.8 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
18:24:06.80 +01:54:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:26:58.99 -05:52:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:27:38.03 -02:35:57.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:29:55.91 -05:58:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:30:06.26 +00:42:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:36:24.26 -03:41:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:37:00.65 -06:14:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:40:10.38 -06:08:15.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:40:13.59 -05:43:15.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:43:25.96 -05:11:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:45:51.57 -05:28:45.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:46:17.00 -06:13:37.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:46:32.18 -02:57:20.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:46:58.12 -04:16:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:47:27.02 -04:13:13.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:47:40.78 -05:38:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:48:44.83 -05:05:53.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:49:52.01 -05:42:04.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:50:04.54 -05:38:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:50:25.00 -05:06:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:50:46.75 -05:02:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:51:17.90 -05:02:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:51:37.37 -03:26:10.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:51:44.49 -05:55:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:52:22.14 -04:33:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:52:24.28 -02:59:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:52:46.46 -01:21:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:52:56.32 -04:06:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:53:20.09 -01:06:45.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:53:28.75 +01:21:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:54:02.33 +00:15:32.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:54:17.87 -05:22:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:54:30.37 -04:23:53.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:55:32.50 -02:28:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:55:40.63 +00:01:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:55:48.92 -01:45:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:56:20.56 -01:56:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:56:27.63 -05:47:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:56:34.08 +00:35:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
18:56:56.21 -01:25:38.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:57:37.27 -05:29:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:57:51.49 +01:23:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:58:03.41 -03:49:01.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:58:09.94 -03:26:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:59:50.33 -01:35:05.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:00:02.75 -03:49:07.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:00:20.12 -02:22:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:00:56.42 -04:12:05.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:01:35.40 -06:13:59.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:01:40.93 +00:14:12.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:02:14.17 -00:19:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:02:41.46 +00:36:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:03:12.03 -03:55:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:03:46.28 -05:55:58.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:03:53.59 -03:41:36.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:05:07.90 -00:11:37.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:05:15.57 +01:54:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:05:19.23 -01:42:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:05:23.30 -03:59:43.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:05:49.50 -01:51:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:06:02.99 -05:49:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:06:11.74 -04:31:52.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:06:28.28 -02:44:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
19:06:40.91 -05:13:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:06:48.21 +01:30:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:06:55.01 -02:33:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:01.34 -05:31:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:10.27 +00:51:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:10.67 -01:04:48.3 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:28.90 -04:16:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:31.27 -05:29:33.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:07:55.14 +00:05:32.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:10.86 -05:28:04.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:12.20 -05:34:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:13.12 -06:12:42.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:24.09 -04:41:30.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:24.24 +01:57:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:26.41 +00:26:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:29.90 -00:27:24.4 -- does not seem to be a hot pixel (will add it to exclusion list)
19:08:39.31 -03:02:06.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:09:00.29 -00:08:19.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:09:17.50 +00:53:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
19:09:21.00 -02:07:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
19:09:24.45 -04:26:51.3 -- 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)
18:24:06.80 +01:54:53.7 -- a known variable star
18:26:58.99 -05:52:13.3 -- a known variable star
18:27:38.03 -02:35:57.1 -- a known variable star
18:29:55.91 -05:58:20.4 -- a known variable star
18:30:06.26 +00:42:33.2 -- a known variable star
18:36:24.26 -03:41:32.2 -- a known variable star
18:37:00.65 -06:14:17.2 -- not a known variable star
18:40:10.38 -06:08:15.7 -- a known variable star
18:40:13.59 -05:43:15.2 -- not a known variable star
18:43:25.96 -05:11:44.3 -- a known variable star
18:45:51.57 -05:28:45.4 -- a known variable star
18:46:17.00 -06:13:37.1 -- a known variable star
18:46:32.18 -02:57:20.9 -- a known variable star
18:46:58.12 -04:16:24.9 -- a known variable star
18:47:27.02 -04:13:13.8 -- a known variable star
18:47:40.78 -05:38:14.9 -- a known variable star
18:48:44.83 -05:05:53.0 -- a known variable star
18:49:52.01 -05:42:04.5 -- a known variable star
18:50:04.54 -05:38:36.8 -- a known variable star
18:50:25.00 -05:06:05.7 -- a known variable star
18:50:46.75 -05:02:07.4 -- a known variable star
18:51:17.90 -05:02:57.4 -- a known variable star
18:51:37.37 -03:26:10.5 -- a known variable star
18:51:44.49 -05:55:51.3 -- a known variable star
18:52:22.14 -04:33:22.1 -- a known variable star
18:52:24.28 -02:59:00.1 -- a known variable star
18:52:46.46 -01:21:21.8 -- not a known variable star
18:52:56.32 -04:06:44.0 -- a known variable star
18:53:20.09 -01:06:45.8 -- not a known variable star
18:53:28.75 +01:21:53.6 -- a known variable star
18:54:02.33 +00:15:32.1 -- a known variable star
18:54:17.87 -05:22:28.8 -- a known variable star
18:54:30.37 -04:23:53.2 -- a known variable star
18:55:32.50 -02:28:48.5 -- a known variable star
18:55:40.63 +00:01:18.9 -- a known variable star
18:55:48.92 -01:45:58.0 -- a known variable star
18:56:20.56 -01:56:14.9 -- a known variable star
18:56:27.63 -05:47:52.3 -- a known variable star
18:56:34.08 +00:35:13.9 -- a known variable star
18:56:56.21 -01:25:38.8 -- a known variable star
18:57:37.27 -05:29:15.1 -- not a known variable star
18:57:51.49 +01:23:37.2 -- not a known variable star
18:58:03.41 -03:49:01.3 -- a known variable star
18:58:09.94 -03:26:39.8 -- a known variable star
18:59:50.33 -01:35:05.2 -- a known variable star
19:00:02.75 -03:49:07.0 -- a known variable star
19:00:20.12 -02:22:05.7 -- a known variable star
19:00:56.42 -04:12:05.4 -- not a known variable star
19:01:35.40 -06:13:59.6 -- a known variable star
19:01:40.93 +00:14:12.9 -- a known variable star
19:02:14.17 -00:19:09.7 -- a known variable star
19:02:41.46 +00:36:11.0 -- a known variable star
19:03:12.03 -03:55:58.3 -- a known variable star
19:03:46.28 -05:55:58.8 -- not a known variable star
19:03:53.59 -03:41:36.2 -- a known variable star
19:05:07.90 -00:11:37.1 -- a known variable star
19:05:15.57 +01:54:04.9 -- a known variable star
19:05:19.23 -01:42:24.8 -- a known variable star
19:05:23.30 -03:59:43.1 -- a known variable star
19:05:49.50 -01:51:55.8 -- a known variable star
19:06:02.99 -05:49:23.1 -- not a known variable star
19:06:11.74 -04:31:52.6 -- a known variable star
19:06:28.28 -02:44:10.0 -- not a known variable star
19:06:40.91 -05:13:22.7 -- a known variable star
19:06:48.21 +01:30:09.4 -- a known variable star
19:06:55.01 -02:33:46.1 -- a known variable star
19:07:01.34 -05:31:54.9 -- not a known variable star
19:07:10.27 +00:51:33.2 -- a known variable star
19:07:10.67 -01:04:48.3 -- a known variable star
19:07:28.90 -04:16:28.7 -- a known variable star
19:07:31.27 -05:29:33.6 -- not a known variable star
19:07:55.14 +00:05:32.5 -- a known variable star
19:08:10.86 -05:28:04.5 -- a known variable star
19:08:12.20 -05:34:52.8 -- not a known variable star
19:08:13.12 -06:12:42.6 -- a known variable star
19:08:24.09 -04:41:30.1 -- a known variable star
19:08:24.24 +01:57:43.2 -- a known variable star
19:08:26.41 +00:26:14.5 -- a known variable star
19:08:29.90 -00:27:24.4 -- not a known variable star
19:08:39.31 -03:02:06.6 -- a known variable star
19:09:00.29 -00:08:19.6 -- a known variable star
19:09:17.50 +00:53:31.1 -- a known variable star
19:09:21.00 -02:07:30.6 -- not a known variable star
19:09:24.45 -04:26:51.3 -- a known variable star
Found 15 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
84 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 84 (excluding asteroids and hot pixels, 15 new), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461140.84018000 -observatory V36
23:38:57.29 -04:50:52.4 Mercury (0.2mag)
02:41:14.52 +15:37:18.0 Venus (-3.9mag)
00:01:44.73 -00:54:30.0 Mars (1.2mag)
07:10:13.87 +22:50:04.7 Jupiter (-2.1mag)
00:26:38.54 +00:33:04.9 Saturn (0.9mag)
03:46:32.05 +19:43:43.7 Uranus (5.8mag)
00:10:05.43 -00:20:06.6 Neptune (7.8mag)
20:33:28.65 -22:52:27.0 Pluto (14.5mag)
19:39:26.37 -25:53:15.7 Moon (-10.3mag)
-rw-r--r-- 1 apache apache 362 Apr 10 04:13 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461140.84018000:
07:10:05.97 +22:50:20.5 Io (5.7mag)
07:10:18.61 +22:49:51.9 Europa (5.9mag)
07:10:09.67 +22:50:05.7 Ganymede (5.3mag)
07:09:54.06 +22:50:51.7 Callisto (6.6mag)
07:13:48.08 +22:40:26.5 Himalia (15.3mag)
07:10:14.70 +22:50:05.2 Thebe (16.2mag)
07:13:51.78 +23:09:59.9 Elara (17.3mag)
07:08:43.64 +23:33:02.7 Pasiphae (17.4mag)
07:18:40.83 +22:47:30.3 Carme (18.5mag)
00:26:48.82 +00:32:56.2 Titan (8.8mag)
00:26:36.56 +00:33:20.9 Rhea (10.1mag)
00:26:29.73 +00:34:06.5 Iapetus (11.5mag)
00:26:52.34 +00:32:54.1 Hyperion (14.8mag)
00:28:19.79 +00:42:28.9 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 10 04:13 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461140.84018000:
15:10:13.79 -11:58:37.8 JWST
19:53:45.90 +03:33:16.3 Chandra
08:29:39.22 -46:38:35.8 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 10 04:13 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461140.84018000 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:49:24.62 -28:27:27.3 13.9mag P/2010 H2 (Vales)
05:02:47.63 -69:56:12.2 17.4mag C/2014 UN271 (Bernardinelli-Bernstein)
05:31:17.93 +31:24:01.7 17.2mag C/2017 K2 (PANSTARRS)
17:30:50.86 +09:52:18.7 17.6mag C/2021 G2 (ATLAS)
23:08:38.11 +29:00:46.9 17.0mag C/2022 E2 (ATLAS)
04:22:41.88 +25:52:55.4 15.9mag C/2022 N2 (PANSTARRS)
09:02:22.64 +31:58:03.4 16.2mag C/2022 QE78 (ATLAS)
08:30:20.10 -00:45:55.9 17.3mag C/2022 R6 (PANSTARRS)
18:54:55.57 +18:03:09.0 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:42:24.17 -11:36:12.2 17.5mag P/2023 B1 (PANSTARRS)
09:10:27.70 -12:48:20.2 17.6mag C/2023 F3 (ATLAS)
21:48:15.13 +62:35:13.5 17.5mag C/2023 H5 (Lemmon)
19:23:41.01 -03:39:06.7 14.2mag C/2023 R1 (PANSTARRS)
21:40:27.14 +85:08:37.4 17.8mag C/2023 X2 (Lemmon)
06:15:37.91 +63:32:47.8 17.1mag C/2024 A1 (ATLAS)
05:00:47.04 +16:16:36.7 10.7mag C/2024 E1 (Wierzchos)
16:22:46.02 +05:27:37.8 17.4mag C/2024 G6 (ATLAS)
20:19:03.72 +13:45:35.8 14.7mag C/2024 J3 (ATLAS)
03:21:20.94 -23:15:39.6 16.4mag C/2024 T5 (ATLAS)
05:12:00.22 +46:43:45.2 17.7mag C/2025 J1 (Borisov)
14:02:18.99 +41:15:34.2 14.9mag C/2025 L1 (ATLAS)
03:16:31.10 -25:21:00.9 17.8mag C/2025 Q3 (ATLAS)
23:07:27.82 +19:41:53.8 9.4mag C/2025 R3 (PANSTARRS)
12:56:34.86 +02:39:38.2 17.5mag C/2025 Y1 (ATLAS)
02:32:01.68 +03:28:03.2 11.0mag C/2026 A1 (MAPS)
23:43:13.88 +36:07:32.5 14.4mag C/2026 B2 (Sun-Gao)
18:31:54.04 -10:00:55.7 12.2mag 10P/Tempel
15:07:47.62 +03:45:39.7 13.5mag 24P/Schaumasse
11:04:25.55 -01:42:56.6 15.7mag 29P/Schwassmann-Wachmann
17:58:53.79 -09:49:34.5 17.8mag 40P/Vaisala
10:38:04.89 -04:34:16.7 16.8mag 43P/Wolf-Harrington
01:39:55.89 +16:31:00.3 17.2mag 47P/Ashbrook-Jackson
07:00:30.96 +38:12:57.2 17.0mag 63P/Wild
23:21:45.94 -12:08:20.4 15.7mag 65P/Gunn
03:48:19.43 +19:15:48.5 15.9mag 76P/West-Kohoutek-Ikemura
00:53:07.25 +07:06:39.7 14.4mag 78P/Gehrels
22:45:38.00 -11:03:38.7 14.6mag 88P/Howell
01:54:32.82 +19:06:27.4 15.1mag 93P/Lovas
04:44:19.25 +31:58:26.3 16.3mag 123P/West-Hartley
08:22:01.64 +40:58:26.5 16.2mag 124P/Mrkos
02:24:31.05 +13:43:57.4 16.4mag 128P/Shoemaker-Holt
02:36:27.90 +13:47:21.3 17.5mag 131P/Mueller
00:56:47.87 +11:12:06.6 10.9mag 141P/Machholz
01:06:25.27 +02:44:49.9 11.0mag 141P-A/Machholz
23:54:37.33 -01:06:03.4 13.5mag 141P-D/Machholz
01:36:09.27 +04:28:11.0 17.9mag 141P-I/Machholz
00:46:37.96 -04:21:42.9 15.2mag 162P/SidingSpring
10:29:48.74 +31:14:26.1 17.9mag 164P/Christensen
06:26:02.82 +24:25:00.7 17.9mag 198P/ODAS
15:01:28.37 -00:41:24.1 17.5mag 210P/Christensen
21:21:59.90 -12:49:03.1 17.5mag 218P/LINEAR
17:14:40.51 -14:36:10.3 16.2mag 235P/LINEAR
05:22:21.85 +34:14:19.7 16.7mag 240P/NEAT
07:35:52.31 -05:47:53.0 17.7mag 242P/Spahr
15:44:41.35 +06:36:20.9 17.5mag 391P/Kowalski
07:32:10.26 +21:20:27.6 17.6mag 450P/LONEOS
05:27:43.15 +45:21:53.0 17.5mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 10 04:13 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 10 04:13 tocp_transients_list.txt
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Truncated list of recent TNS transients from https://www.wis-tns.org/ :
09:56:30.436 -12:41:18.06 AT 2026ikg 2026-03-22.44 20.38
09:24:18.822 -19:21:24.31 AT 2026ikf 2026-03-25.57 19.79
08:18:48.927 -23:32:12.08 AT 2026ike 2026-02-12.51 20.2
08:47:41.490 -21:46:40.10 AT 2026ikd 2026-03-28.41 19.49
08:34:30.248 -07:09:24.85 AT 2026ikc 2026-03-29.44 19.28
13:21:25.078 +79:09:18.53 AT 2026ikb 2026-03-25.43 20.7322
09:05:18.124 -19:48:21.41 AT 2026ika 2026-03-09.36 20.58
08:38:25.468 +06:11:03.79 AT 2026ijz 2026-03-09.32 21.99
08:00:34.010 +04:48:18.04 AT 2026ijy 2026-03-09.31 21.07
09:02:07.082 +07:27:03.87 AT 2026ijx 2026-02-17.43 21.29
10:37:20.784 +30:59:50.95 AT 2026ijw 2026-03-10.33 20.2
16:00:37.915 +06:38:30.61 AT 2026ijv 2026-03-28.57 20.5
13:51:30.137 +25:53:04.17 AT 2026iju 2026-03-28.41 20.07
12:52:01.341 -19:06:48.80 AT 2026ijt 2026-01-28.59 20.22
11:38:25.995 -11:34:40.48 AT 2026ijs 2026-01-16.56 21.1
07:12:41.661 +56:25:20.59 AT 2026ijr 2026-01-19.40 20.76
09:34:48.813 +06:57:40.76 AT 2026ijq 2026-01-26.43 21.57
10:49:59.384 +25:17:19.22 AT 2026ijp 2026-04-04.17 19.836
08:20:22.449 +03:44:22.06 AT 2026ijo 2026-04-02.18 19.8276
06:41:34.987 -19:08:36.17 AT 2026ijn 2026-02-05.26 20.38
-rw-r--r-- 1 apache apache 30K Apr 10 04:13 tns_transients_list.txt