This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.3769* 18 11 32.11 -14 28 56.2 10.4 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J181132-1428.9,2461132.8769,10.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J181132-1428.9 20260402.3769 10.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4119548363344273152,2461132.8769,10.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4119548363344273152 20260402.3769 10.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4095080415704838784,2461132.8769,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4095080415704838784 20260402.3769 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J267.8249-16.0651,2461132.8769,13.09,0.05,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 J267.8249-16.0651 20260402.3769 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4119344300921411712,2461132.8769,12.73,0.05,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
Gaia DR3 4119344300921411712 20260402.3769 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J272.9053-16.8478,2461132.8769,11.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J272.9053-16.8478 20260402.3769 11.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.3769* 18 10 57.14 -14 29 13.3 10.5 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4146877102842918528,2461132.8769,10.54,0.05,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
Gaia DR3 4146877102842918528 20260402.3769 10.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.3769* 18 10 42.08 -15 27 27.1 12.3 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4146004331095322496,2461132.8769,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4146004331095322496 20260402.3769 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461132.8769,13.01,0.05,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
VARIABLE_NAME 20260402.3769 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!
TCP 2026 04 02.3769* 18 11 38.92 -15 26 11.0 12.7 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J181139.48-152605.4,2461132.8769,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J181139.48-152605.4 20260402.3769 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 04 02.3769 2461132.8769 13.16 18:10:51.68 -13:54:18.0
15.94837 2.44023 galactic Ser Second-epoch detections are separated by 1.9" and 1.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 4147333984253955584 | 18:10:52.09 -13:54:12.8 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.3769* 18 10 51.68 -13 54 18.0 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 4147333984253955584,2461132.8769,13.16,0.05,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
Large-amplitude variable Gaia DR2 4147333984253955584 20260402.3769 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J181040.85-160150.2,2461132.8769,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J181040.85-160150.2 20260402.3769 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VV Sgr,2461132.8769,12.37,0.05,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
VV Sgr 20260402.3769 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!
TCP 2026 04 02.3769* 18 09 53.55 -14 36 26.2 11.9 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J180953.87-143623.0,2461132.8769,11.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J180953.87-143623.0 20260402.3769 11.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.3769* 18 08 24.06 -15 03 29.5 12.7 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4146830403633533568,2461132.8769,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4146830403633533568 20260402.3769 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.3769* 18 06 42.95 -14 19 09.5 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4146932142812692992,2461132.8769,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4146932142812692992 20260402.3769 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J173249-2142.0,2461132.8769,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J173249-2142.0 20260402.3769 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4145662825357917184,2461132.8769,10.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4145662825357917184 20260402.3769 10.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4095593922006889344,2461132.8769,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4095593922006889344 20260402.3769 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.3769* 18 02 04.59 -15 03 18.6 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J180204.85-150315.7,2461132.8769,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J180204.85-150315.7 20260402.3769 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J180821.33-180434.5,2461132.8769,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J180821.33-180434.5 20260402.3769 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.3769* 18 05 28.56 -14 14 20.7 11.6 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4147119678265478912,2461132.8769,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4147119678265478912 20260402.3769 11.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.3769* 18 01 11.67 -15 20 33.3 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4145459072117841024,2461132.8769,12.48,0.05,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
Gaia DR3 4145459072117841024 20260402.3769 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J175450.86-213712.7,2461132.8769,12.61,0.05,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 J175450.86-213712.7 20260402.3769 12.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.3769* 17 24 20.13 -15 27 08.0 12.9 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J172420-1527.2,2461132.8769,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J172420-1527.2 20260402.3769 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J272.5214-16.0282,2461132.8769,11.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J272.5214-16.0282 20260402.3769 11.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J174832.78-210623.0,2461132.8769,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 J174832.78-210623.0 20260402.3769 12.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 02.3769* 18 08 37.46 -15 06 17.6 12.4 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4146079231038031360,2461132.8769,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4146079231038031360 20260402.3769 12.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J265.5784-18.0506,2461132.8769,12.71,0.05,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
ATO J265.5784-18.0506 20260402.3769 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0554 Oph,2461132.8769,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0554 Oph 20260402.3769 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J260.4137-20.5400,2461132.8769,12.53,0.05,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 J260.4137-20.5400 20260402.3769 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J180901.40-191852.1,2461132.8769,11.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J180901.40-191852.1 20260402.3769 11.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461099.00589001 27.02.2026 12:08:18.897 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
First image: 2461099.00589001 27.02.2026 12:08:18.897 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
Last image: 2461132.87711758 02.04.2026 09:02:52.959 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 32
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.23
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 10152
Objects passed selection criteria: 10129
Measurements per detected object (mean, median, min, max): 3.0 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 4.0 2 4
Average stars detected per image: 8129
Average stars matched: 7904 (97.2321 %)
Memory usage VmPeak: 117052 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 1 15:05:04 CDT 2026
VaST build number 1.0rc88-372-gf0c1109d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-01)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 2 04:13:59 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: 2461099.00589001 27.02.2026 12:08:18.897 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
First image: 2461099.00589001 27.02.2026 12:08:18.897 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
Last image: 2461132.87711758 02.04.2026 09:02:52.959 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 400
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.87
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: 39 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): 134772
Objects passed selection criteria: 134448
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 103556
Average stars matched: 98644.5 (95.2569 %)
Memory usage VmPeak: 2089352 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 1 15:05:04 CDT 2026
VaST build number 1.0rc88-372-gf0c1109d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-01)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 2 04:18:00 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/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits
SExtractor catalog cache: saved Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat to cache
SExtractor catalog cache: saved Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.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/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461132.87662608
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_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits exists and is non-empty
Saving wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits to local_wcs_cache/
'wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits' -> 'local_wcs_cache/wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits'
wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits exists and is non-empty
Saving wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits to local_wcs_cache/
'wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits' -> 'local_wcs_cache/wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits'
wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits exists and is non-empty
Saving wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits to local_wcs_cache/
'wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits' -> 'local_wcs_cache/wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits'
wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits exists and is non-empty
Saving wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits to local_wcs_cache/
'wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits' -> 'local_wcs_cache/wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.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 17:46:18.174 -18:00:45.70
Second-epoch image center 17:46:55.965 -18:00:41.29
Angular distance between the image centers 0.15 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 17:46:18.174 -18:00:45.70
Second-epoch image center 17:46:55.578 -18:00:47.84
Angular distance between the image centers 0.15 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 17:46:55.965 -18:00:41.29
Second-epoch second image center 17:46:55.578 -18:00:47.84
Angular distance between the image centers 0.00238 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/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits &> /tmp/tmp.6VoiGOcaNQ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits &> /tmp/tmp.bLqLF9LRMF
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits &> /tmp/tmp.5jCg3da8s2
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits &> /tmp/tmp.OcS6BNsGIp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits
Calibrating the magnitude scale
Found non-empty wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.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_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits and wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.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_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits and wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat
Found non-empty wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits and wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat
The reference image (wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits) and catalog (wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat) found
'wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat' -> 'wcsmag.cat'
Read 15752 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 258.0365 to 275.0296 deg, Dec -23.3066 to -12.5656 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 258.0365 to 275.0296 deg, Dec -23.3066 to -12.5656 deg
Loaded 14544 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): 9713 out of 10414 total matches.
Matched with Tycho-2 10414 out of 15752 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.846952
a=0.000000 b=1.000000 c=22.846952
From vast_summary.log: estimated ref. image limiting mag.: -8.23
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.62
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.62
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 7 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
2.3 pix Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
3.0 pix fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits
3.0 pix fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits
Limiting magnitude estimates:
14.6 mag. Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
14.6 mag. Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
13.7 mag. fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits
13.7 mag. fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits
All-image limiting magnitude estimate: 13.7 (SNR ) 11.1 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.6VoiGOcaNQ (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/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits' -> 'wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
WCS_IMAGE_NAME=wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
WCS-calibrated image found: wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
Checking if the catalog wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat corresponding to the image wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits alredy exist and is non-empty...
Catalog wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat corresponding to the image wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
WCS catalog name: wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1456, passed=15752
Got 15752 stars (including 14271 good ones) from the SExtractor catalog wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat
util/solve_plate_with_UCAC5 got 15752 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 919 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
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 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 918 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.37"
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 914 stars left (next iteration limit 1006)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits -region wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.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.bLqLF9LRMF (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/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits' -> 'wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
WCS_IMAGE_NAME=wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
WCS-calibrated image found: wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
Checking if the catalog wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat corresponding to the image wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits alredy exist and is non-empty...
Catalog wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat corresponding to the image wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
WCS catalog name: wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1474, passed=15602
Got 15602 stars (including 14101 good ones) from the SExtractor catalog wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat
util/solve_plate_with_UCAC5 got 15602 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 919 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
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 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 918 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.39"
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 915 stars left (next iteration limit 1007)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits -region wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.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.5jCg3da8s2 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits
WCS-calibrated image found: wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits
Checking if the catalog wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits.cat corresponding to the image wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits.cat corresponding to the image wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits
WCS catalog name: wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=506, passed=6979
Got 6979 stars (including 6470 good ones) from the SExtractor catalog wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits.cat
util/solve_plate_with_UCAC5 got 6979 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 914 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.99"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.94"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 914 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.97"
Estimated accuracy of the plate solution: 1.14"
Excluding outliers - 907 stars left (next iteration limit 997)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits -region wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.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.OcS6BNsGIp (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits
WCS-calibrated image found: wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits
Checking if the catalog wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits.cat corresponding to the image wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits.cat corresponding to the image wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits
WCS catalog name: wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=518, passed=7005
Got 7005 stars (including 6484 good ones) from the SExtractor catalog wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits.cat
util/solve_plate_with_UCAC5 got 7005 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 914 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.99"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.96"
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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 914 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.98"
Estimated accuracy of the plate solution: 1.19"
Excluding outliers - 907 stars left (next iteration limit 997)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits -region wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.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_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits'
Saving fully-calibrated image wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits'
Saving fully-calibrated image wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits'
Saving fully-calibrated image wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits'
Preparing the HTML report for the field Sgr-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20827.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20846.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out20810.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20842.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20750_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 20750_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:11:41.42 -16:04:42.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20810_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
Preparing report for the candidate 20810_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20813_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 20813_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:10:57.20 -14:29:12.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20827_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 20827_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:10:59.20 -13:38:31.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.60, MAG_FAINT_SEARCH_LIMIT=11.58)GAIADR2_OUTPUT=# 5.475 4147365831431437696 272.74778010211 -13.64095912733 9.7778 8.5551 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.475#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20842_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
Preparing report for the candidate 20842_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20846_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 20846_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:11:33.23 -13:43:34.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.84, MAG_FAINT_SEARCH_LIMIT=11.82)GAIADR2_OUTPUT=# 4.996 4147360544333566080 272.88941537371 -13.72533085338 10.2467 9.1654 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.996#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06388_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 06388_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:11:57.27 -18:52:14.0 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 7s
Prepared the HTML report for the field Sgr-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
18:11:32.11 -14:28:56.2
17:53:52.37 -19:07:47.2
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/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits
SExtractor catalog cache: saved Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat to cache
SExtractor catalog cache: saved Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
Creating symlink local_wcs_cache/wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
Creating symlink local_wcs_cache/wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits
Creating symlink local_wcs_cache/wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.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_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits exists and is non-empty
wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits exists and is non-empty
wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits exists and is non-empty
wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.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 17:46:18.174 -18:00:45.70
Second-epoch image center 17:46:55.965 -18:00:41.29
Angular distance between the image centers 0.15 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 17:46:18.174 -18:00:45.70
Second-epoch image center 17:46:55.578 -18:00:47.84
Angular distance between the image centers 0.15 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 17:46:55.965 -18:00:41.29
Second-epoch second image center 17:46:55.578 -18:00:47.84
Angular distance between the image centers 0.00238 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/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits &> /tmp/tmp.gRNZRDvpUJ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits &> /tmp/tmp.GaB5EsldFS
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits &> /tmp/tmp.xkLxEj7O4O
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits &> /tmp/tmp.k2jSU2I36b
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits
Calibrating the magnitude scale
Found non-empty wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.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_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits and wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.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_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits and wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat
Found non-empty wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits and wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat
The reference image (wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits) and catalog (wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat) found
'wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat' -> 'wcsmag.cat'
Read 179796 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 258.0045 to 275.0499 deg, Dec -23.3098 to -12.5486 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 258.0045 to 275.0499 deg, Dec -23.3098 to -12.5486 deg
Loaded 14601 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): 9967 out of 12785 total matches.
Matched with Tycho-2 12785 out of 179796 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.613163
a=0.000000 b=1.000000 c=22.613163
From vast_summary.log: estimated ref. image limiting mag.: -7.87
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.74
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.74
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 170 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
1.9 pix Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
2.5 pix fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits
2.5 pix fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits
Limiting magnitude estimates:
14.7 mag. Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
14.7 mag. Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
13.8 mag. fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits
13.8 mag. fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 13.2 (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.gRNZRDvpUJ (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/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits' -> 'wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
WCS_IMAGE_NAME=wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
WCS-calibrated image found: wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
Checking if the catalog wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat corresponding to the image wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits alredy exist and is non-empty...
Catalog wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat corresponding to the image wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
WCS catalog name: wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=28, blended=17851, passed=179768
Got 179768 stars (including 161620 good ones) from the SExtractor catalog wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat
util/solve_plate_with_UCAC5 got 179768 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 923 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 923 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.41"
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 919 stars left (next iteration limit 1012)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits -region wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.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.GaB5EsldFS (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/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits' -> 'wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
WCS_IMAGE_NAME=wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
WCS-calibrated image found: wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
Checking if the catalog wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat corresponding to the image wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits alredy exist and is non-empty...
Catalog wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat corresponding to the image wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
WCS catalog name: wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=17987, passed=181054
Got 181054 stars (including 162799 good ones) from the SExtractor catalog wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat
util/solve_plate_with_UCAC5 got 181054 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 925 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 924 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.45"
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 921 stars left (next iteration limit 1013)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits -region wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.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.xkLxEj7O4O (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits
WCS-calibrated image found: wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits
Checking if the catalog wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits.cat corresponding to the image wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits.cat corresponding to the image wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits
WCS catalog name: wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=4853, passed=63452
Got 63452 stars (including 58556 good ones) from the SExtractor catalog wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits.cat
util/solve_plate_with_UCAC5 got 63452 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 923 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.91"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.80"
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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 923 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.80"
Estimated accuracy of the plate solution: 0.92"
Excluding outliers - 915 stars left (next iteration limit 1006)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits -region wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.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.k2jSU2I36b (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits
WCS-calibrated image found: wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits
Checking if the catalog wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits.cat corresponding to the image wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits.cat corresponding to the image wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits
WCS catalog name: wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=4733, passed=63472
Got 63472 stars (including 58697 good ones) from the SExtractor catalog wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits.cat
util/solve_plate_with_UCAC5 got 63472 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 922 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.88"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.77"
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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 922 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.77"
Estimated accuracy of the plate solution: 0.89"
Excluding outliers - 916 stars left (next iteration limit 1005)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits -region wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.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_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/wcs_Sgr-01-Q2b1x1_2026-02-27_06-08-18_20.00sec_-15.00C_LIGHT_0061.fits
Saving fully-calibrated image wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/wcs_Sgr-01-Q2b1x1_2026-02-27_06-09-19_20.00sec_-15.00C_LIGHT_0062.fits
Saving fully-calibrated image wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-10_20.00sec_-15.00C_LIGHT_0031.fits
Saving fully-calibrated image wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-01-Q2b1x1_040853_TTUQ2b1x1_30242_BcwGFJs0/wcs_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032.fits
Preparing the HTML report for the field Sgr-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out139764.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out191749.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208311.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208319.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208326.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208327.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208331.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208336.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208342.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208346.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208349.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208354.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208360.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208371.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208374.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208465.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208497.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208573.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208579.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208781.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208811.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208913.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out208949.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out209034.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out209043.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out209089.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out209212.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out209225.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out209239.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out209249.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out209254.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out70901.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out208337.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out208897.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out209175.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out123322.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out126820.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out127023.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out129899.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out130199.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132539.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133191.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133769.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137734.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out142924.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out173626.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20322.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out208318.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out208320.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out208356.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out208383.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out208459.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out208899.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out209055.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out209068.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out209247.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out22418.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out23872.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out29870.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35707.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56756.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out56976.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out74429.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82938.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out83425.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 31s
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: 15s
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Considering the candidate 208311_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208311_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:43:48.10 -16:26:49.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 1.747 4124083707073175040 265.95081499632 -16.44738253732 12.8729 11.7829 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.747#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 208318_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
Preparing report for the candidate 208318_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
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Considering the candidate 208319_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208319_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:00:11.85 -16:00:28.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 4.629 4145120770518506752 270.04851674988 -16.00876409857 13.0156 11.8539 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.629#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 208320_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
Preparing report for the candidate 208320_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
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Considering the candidate 208324_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208324_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:44:37.30 -15:23:11.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 208325_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208325_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:11:04.17 -16:36:14.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 208326_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208326_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:05:08.52 -14:30:31.4 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 208327_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208327_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:07:31.15 -15:30:32.8 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 208331_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208331_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:19:15.37 -20:49:54.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 3.579 4115910148126157824 259.81498278707 -20.83221309152 12.9679 11.9904 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.579#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 208336_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208336_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:10:17.67 -18:06:00.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 3.390 4095806299538356480 272.57449671529 -18.10061423310 12.5299 12.1158 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.390#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 208337_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208337_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:10:19.84 -15:50:01.5 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)
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Considering the candidate 208339_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208339_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:52:17.17 -18:04:36.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 208342_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208342_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:00:16.65 -16:16:25.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.75, MAG_FAINT_SEARCH_LIMIT=13.73)
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Considering the candidate 208346_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208346_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:37:42.59 -15:50:38.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 3.771 4124869999694546560 264.42852391560 -15.84424365215 12.8272 12.1290 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.771#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 208349_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208349_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:44:11.71 -20:16:56.9 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 208352_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208352_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 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 208354_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208354_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:11:18.67 -16:33:32.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.58, MAG_FAINT_SEARCH_LIMIT=13.56)
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Considering the candidate 208356_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
Preparing report for the candidate 208356_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
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Considering the candidate 208360_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208360_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:56:25.00 -22:01:30.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)
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Considering the candidate 208367_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208367_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:59:47.89 -20:13:17.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 208371_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208371_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:43:00.04 -20:56:24.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 1.508 4117409160513963776 265.75017213538 -20.94050229094 11.5542 10.1498 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.508#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 208372_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208372_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 208374_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208374_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:44:38.02 -13:45:48.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 1.399 4149425972623748352 266.15842299487 -13.76394408913 12.6831 12.4907 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.399#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 208376_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208376_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:53:05.31 -13:59:15.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 208377_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208377_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:20:34.66 -20:44:11.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 208379_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208379_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:18:10.72 -19:51:14.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 208383_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
Preparing report for the candidate 208383_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208390_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208390_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:17:59.75 -21:57:28.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 208391_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208391_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:05:19.15 -14:19:16.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 208393_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208393_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:11:41.46 -16:04:41.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 208395_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208395_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:11:51.06 -15:40:45.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 208434_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208434_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:11:01.34 -14:14:26.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 208453_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208453_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:11:32.06 -14:28:56.8 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 208459_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
Preparing report for the candidate 208459_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208465_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208465_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:10:59.18 -13:38:31.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.62, MAG_FAINT_SEARCH_LIMIT=11.60)GAIADR2_OUTPUT=# 5.823 4147365831431437696 272.74778010211 -13.64095912733 9.7778 8.5551 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.823#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208482_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208482_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:53:52.36 -19:07:47.3 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208497_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208497_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:11:33.22 -13:43:34.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.88, MAG_FAINT_SEARCH_LIMIT=11.86)GAIADR2_OUTPUT=# 5.095 4147360544333566080 272.88941537371 -13.72533085338 10.2467 9.1654 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.095#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208535_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208535_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:11:09.74 -14:13:11.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208548_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208548_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:37:26.68 -15:24:56.1 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208573_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208573_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:11:02.57 -13:57:58.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.39, MAG_FAINT_SEARCH_LIMIT=12.37)GAIADR2_OUTPUT=# 1.024 4147286396018914944 272.76095139212 -13.96620208743 11.0055 10.1843 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.024#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208579_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208579_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:10:42.09 -13:48:36.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.45, MAG_FAINT_SEARCH_LIMIT=12.43)GAIADR2_OUTPUT=# 3.086 4147338622820585216 272.67599586119 -13.80941826056 10.8459 9.7991 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.086#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208697_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208697_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:25:59.50 -14:03:15.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 208720_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208720_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:29:59.53 -17:21:56.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208748_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208748_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:11:39.01 -13:54:29.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208781_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208781_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:19:03.15 -18:32:52.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208807_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208807_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:11:47.47 -15:11:23.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 208811_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208811_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:10:23.17 -13:36:41.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.17, MAG_FAINT_SEARCH_LIMIT=13.15)GAIADR2_OUTPUT=# 1.657 4147376998346406784 272.59672579202 -13.61099261816 11.7370 10.8250 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.657#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208826_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208826_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:23:35.75 -16:44:00.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208868_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208868_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:19:52.33 -17:46:29.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208879_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208879_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:11:25.20 -13:57:56.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208897_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208897_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:10:27.18 -14:00:45.6 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208899_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
Preparing report for the candidate 208899_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208913_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208913_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:10:41.52 -13:41:12.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 2.819 4147363842868658944 272.67374501861 -13.68647918253 12.0514 11.1461 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.819#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208922_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208922_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:41:30.67 -16:24:32.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 208944_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208944_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:37:09.44 -20:29:59.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208949_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208949_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:11:23.49 -13:47:54.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.41, MAG_FAINT_SEARCH_LIMIT=13.39)GAIADR2_OUTPUT=# 2.275 4147358482749231104 272.84846888473 -13.79807478063 11.9887 11.1380 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.275#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208954_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208954_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:35:38.46 -14:39:26.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208980_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208980_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:23:37.60 -16:00:55.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208992_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208992_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:35:14.53 -14:20:39.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 208994_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 208994_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:11:18.44 -14:03:29.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 209004_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 209004_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:56:25.65 -16:13:47.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 209008_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 209008_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:11:17.54 -14:00:26.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 209034_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 209034_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:11:13.28 -13:36:20.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 2.561 4147366209388559104 272.80605869876 -13.60565530798 12.1996 11.2969 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.561#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 209043_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 209043_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:42:10.42 -15:43:15.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 209055_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
Preparing report for the candidate 209055_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 209068_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
Preparing report for the candidate 209068_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 209089_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 209089_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:04:40.89 -15:13:24.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 1.447 4146763715713355136 271.17044892147 -15.22392344341 11.8515 10.3197 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.447#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 209098_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 209098_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:11:43.27 -14:29:32.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 209112_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 209112_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:01:12.82 -15:19:55.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 209127_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 209127_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:27:00.50 -18:23:14.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 209131_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 209131_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:25:14.58 -18:35:25.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 209133_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 209133_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:36:56.35 -19:47:50.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209134_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 209134_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:29:32.91 -20:22:01.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209148_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 209148_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:02:53.96 -14:31:51.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209170_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 209170_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:11:56.08 -16:32:31.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209172_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 209172_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:34:56.97 -15:44:34.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209175_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 209175_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:10:47.40 -14:25:15.4 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)
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Considering the candidate 209181_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 209181_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:20:56.68 -19:10:05.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209187_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 209187_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 209199_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 209199_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:54:56.00 -15:21:11.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209201_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 209201_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:38:00.92 -15:21:44.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209202_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 209202_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:26:31.99 -15:08:52.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209212_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 209212_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:09:42.02 -13:42:13.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 4.007 4147354217840847104 272.42599780069 -13.70319077370 12.2931 11.1091 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.007#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 209214_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 209214_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:43:19.82 -14:59:06.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209225_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 209225_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:35:39.04 -14:42:21.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 0.905 4137276132943247104 263.91289574607 -14.70585324934 13.6387 11.6280 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.905#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 209231_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 209231_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:42:39.55 -19:31:35.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209232_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 209232_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:09:21.71 -16:17:17.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209239_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 209239_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:43:11.33 -15:00:38.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 3.895 4149047641908967168 265.79629154329 -15.01137157686 12.7561 11.4794 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.895#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 209247_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
Preparing report for the candidate 209247_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
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Considering the candidate 209249_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 209249_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:04:28.39 -18:57:41.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.25, MAG_FAINT_SEARCH_LIMIT=14.23)GAIADR2_OUTPUT=# 3.670 4095394669879067904 271.11916019158 -18.96097940982 12.2745 10.2990 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.670#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 209250_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 209250_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:40:16.34 -15:05:02.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209254_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 209254_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:41:27.51 -14:27:39.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 1.073 4149278539328716544 265.36438739139 -14.46121719345 13.5873 12.8288 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.073#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 209261_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 209261_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:37:26.99 -18:14:22.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 209265_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 209265_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 209267_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 209267_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 106388_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 106388_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:11:06.73 -16:59:48.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 126820_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
Preparing report for the candidate 126820_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
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Considering the candidate 128344_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 128344_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:10:04.53 -15:57:44.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 84473_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 84473_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:11:21.19 -17:58:13.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 142858_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 142858_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:57:09.44 -15:34:54.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197834_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 197834_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:56:17.13 -16:53:24.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 60437_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 60437_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:38:29.58 -19:05:54.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33957_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 33957_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:20:59.04 -20:38:46.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56976_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
Preparing report for the candidate 56976_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
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Considering the candidate 191506_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 191506_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:18:14.72 -21:44:27.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 139764_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 139764_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:10:08.69 -15:18:42.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.63, MAG_FAINT_SEARCH_LIMIT=11.61)GAIADR2_OUTPUT=# 2.218 4146058310295871616 272.53593358184 -15.31233389112 10.4365 10.2947 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.218#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 44480_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 44480_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:21:49.44 -19:58:58.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 173626_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
Preparing report for the candidate 173626_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
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Considering the candidate 194022_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 194022_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:08:24.20 -15:02:36.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57309_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 57309_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:09:51.55 -19:16:40.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 111310_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 111310_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:48:11.36 -16:47:20.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 140816_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 140816_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:09:17.68 -15:27:51.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 133191_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
Preparing report for the candidate 133191_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
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Considering the candidate 179667_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 179667_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:10:26.62 -15:00:16.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 146870_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 146870_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:28:22.94 -15:40:47.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130199_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
Preparing report for the candidate 130199_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
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Considering the candidate 113772_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 113772_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:41:12.47 -16:39:42.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 178698_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 178698_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:44:10.72 -14:56:06.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65527_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 65527_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:11:57.23 -18:52:14.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 120701_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 120701_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:42:00.30 -16:20:48.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20322_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
Preparing report for the candidate 20322_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
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Considering the candidate 85879_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 85879_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:04:15.03 -17:56:38.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192011_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 192011_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:11:39.90 -19:22:03.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 192007_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 192007_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:11:11.66 -19:29:50.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191765_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 191765_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:56:09.55 -20:47:21.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191749_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 191749_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:08:35.90 -18:45:21.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.42, MAG_FAINT_SEARCH_LIMIT=13.40)GAIADR2_OUTPUT=# 4.973 4095743348191759232 272.15095465389 -18.75652654526 11.6748 10.3867 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.973#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191720_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 191720_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:08:45.97 -16:26:01.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 191679_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 191679_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:59:33.68 -18:31:47.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 90291_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 90291_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:29:56.33 -17:40:41.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 123322_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
Preparing report for the candidate 123322_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 135786_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 135786_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:09:52.66 -15:12:13.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 190967_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 190967_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:31:56.07 -19:19:43.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136842_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 136842_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:02:00.58 -15:16:33.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74429_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
Preparing report for the candidate 74429_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21013_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 21013_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:28:52.99 -21:36:59.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129825_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 129825_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:10:44.21 -14:11:41.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 132539_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
Preparing report for the candidate 132539_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 162656_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 162656_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:46:30.69 -13:45:43.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 49619_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 49619_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:19:07.90 -19:36:03.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 119291_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 119291_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:07:48.51 -16:24:22.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136162_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 136162_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:23:47.15 -15:06:52.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 59063_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 59063_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:11:57.46 -19:10:07.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 197668_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 197668_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:19:42.28 -14:55:11.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 82938_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
Preparing report for the candidate 82938_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 179162_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 179162_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:09:28.13 -14:58:10.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129899_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
Preparing report for the candidate 129899_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137734_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
Preparing report for the candidate 137734_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104635_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 104635_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:24:29.02 -16:58:42.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103662_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 103662_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:11:45.18 -17:06:53.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 168505_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 168505_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:11:38.80 -14:07:52.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22418_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
Preparing report for the candidate 22418_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 142924_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
Preparing report for the candidate 142924_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 70901_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 70901_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:37:39.74 -18:34:37.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 2.259 4123158674198631552 264.41531036755 -18.57762720435 12.8217 11.1405 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.259#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 49659_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 49659_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:24:39.67 -19:39:41.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 127023_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
Preparing report for the candidate 127023_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 29870_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
Preparing report for the candidate 29870_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32153_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 32153_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:18:19.77 -20:43:33.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133769_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
Preparing report for the candidate 133769_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 83425_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
Preparing report for the candidate 83425_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 195040_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 195040_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:43:29.48 -14:52:28.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 23872_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
Preparing report for the candidate 23872_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 104400_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 104400_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:11:11.82 -17:05:28.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35707_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
Preparing report for the candidate 35707_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 56756_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
Preparing report for the candidate 56756_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 129792_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 129792_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:11:46.73 -15:52:54.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 175775_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 175775_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:21:15.19 -14:38:04.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 172062_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 172062_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:10:53.68 -14:26:49.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 148434_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 148434_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:11:47.61 -15:48:18.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25679_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 25679_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 17:19:58.08 -21:11:41.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 178312_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032
The candidate 178312_fd_Sgr-01-Q2b1x1_2026-04-02_04-02-52_20.00sec_-15.00C_LIGHT_0032 did not pass the final checks
**** FOUND 18:10:51.82 -14:53:58.3 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 3s
make_report_in_HTML.sh TOTAL: 49s
Prepared the HTML report for the field Sgr-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
18:11:32.11 -14:28:56.2
17:53:52.37 -19:07:47.2
18:10:09.39 -16:12:28.8
18:10:40.34 -16:01:51.8
18:10:04.85 -16:01:42.4
18:05:28.56 -14:14:20.7
18:06:42.95 -14:19:09.5
18:02:04.59 -15:03:18.6
18:08:24.06 -15:03:29.5
18:08:37.46 -15:06:17.6
18:01:11.67 -15:20:33.3
17:24:20.13 -15:27:08.0
18:09:53.55 -14:36:26.2
17:32:49.11 -21:41:59.0
18:09:24.82 -19:33:59.0
17:51:18.15 -16:03:55.5
17:55:40.90 -19:20:49.8
18:11:38.21 -16:51:28.1
18:10:57.14 -14:29:13.3
18:10:42.08 -15:27:27.1
17:20:12.11 -18:46:51.3
18:11:38.92 -15:26:11.0
18:10:51.68 -13:54:18.0
17:54:50.72 -21:37:11.0
17:42:51.28 -21:30:11.3
17:48:32.71 -21:06:21.7
17:21:39.51 -20:32:06.4
18:09:01.00 -19:18:52.1
17:57:02.79 -19:20:16.3
18:11:26.78 -18:24:59.0
18:08:20.91 -18:04:34.2
17:42:19.25 -18:03:02.9
########### Completed Sgr-01-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
18:11:32.11 -14:28:56.2
17:53:52.37 -19:07:47.2
18:09:24.82 -19:33:59.0
17:51:18.15 -16:03:55.5
17:55:40.90 -19:20:49.8
18:11:38.21 -16:51:28.1
18:10:57.14 -14:29:13.3
18:10:42.08 -15:27:27.1
17:20:12.11 -18:46:51.3
18:11:38.92 -15:26:11.0
18:10:51.68 -13:54:18.0
18:10:40.34 -16:01:51.8
17:57:02.79 -19:20:16.3
18:09:53.55 -14:36:26.2
18:08:24.06 -15:03:29.5
18:06:42.95 -14:19:09.5
17:32:49.11 -21:41:59.0
18:10:09.39 -16:12:28.8
18:11:26.78 -18:24:59.0
18:02:04.59 -15:03:18.6
18:08:20.91 -18:04:34.2
18:05:28.56 -14:14:20.7
18:01:11.67 -15:20:33.3
17:54:50.72 -21:37:11.0
17:24:20.13 -15:27:08.0
18:10:04.85 -16:01:42.4
17:48:32.71 -21:06:21.7
18:08:37.46 -15:06:17.6
17:42:19.25 -18:03:02.9
17:42:51.28 -21:30:11.3
17:21:39.51 -20:32:06.4
18:09:01.00 -19:18:52.1
###################################################################################
18:11:32.11 -14:28:56.2 -- not an asteroid (will add it to exclusion list)
17:53:52.37 -19:07:47.2 -- asteroid (will NOT add it to exclusion list)
18:09:24.82 -19:33:59.0 -- not an asteroid (will add it to exclusion list)
17:51:18.15 -16:03:55.5 -- not an asteroid (will add it to exclusion list)
17:55:40.90 -19:20:49.8 -- not an asteroid (will add it to exclusion list)
18:11:38.21 -16:51:28.1 -- not an asteroid (will add it to exclusion list)
18:10:57.14 -14:29:13.3 -- not an asteroid (will add it to exclusion list)
18:10:42.08 -15:27:27.1 -- not an asteroid (will add it to exclusion list)
17:20:12.11 -18:46:51.3 -- asteroid (will NOT add it to exclusion list)
18:11:38.92 -15:26:11.0 -- not an asteroid (will add it to exclusion list)
18:10:51.68 -13:54:18.0 -- not an asteroid (will add it to exclusion list)
18:10:40.34 -16:01:51.8 -- not an asteroid (will add it to exclusion list)
17:57:02.79 -19:20:16.3 -- not an asteroid (will add it to exclusion list)
18:09:53.55 -14:36:26.2 -- not an asteroid (will add it to exclusion list)
18:08:24.06 -15:03:29.5 -- not an asteroid (will add it to exclusion list)
18:06:42.95 -14:19:09.5 -- not an asteroid (will add it to exclusion list)
17:32:49.11 -21:41:59.0 -- not an asteroid (will add it to exclusion list)
18:10:09.39 -16:12:28.8 -- not an asteroid (will add it to exclusion list)
18:11:26.78 -18:24:59.0 -- not an asteroid (will add it to exclusion list)
18:02:04.59 -15:03:18.6 -- not an asteroid (will add it to exclusion list)
18:08:20.91 -18:04:34.2 -- not an asteroid (will add it to exclusion list)
18:05:28.56 -14:14:20.7 -- not an asteroid (will add it to exclusion list)
18:01:11.67 -15:20:33.3 -- not an asteroid (will add it to exclusion list)
17:54:50.72 -21:37:11.0 -- not an asteroid (will add it to exclusion list)
17:24:20.13 -15:27:08.0 -- asteroid (will NOT add it to exclusion list)
18:10:04.85 -16:01:42.4 -- not an asteroid (will add it to exclusion list)
17:48:32.71 -21:06:21.7 -- not an asteroid (will add it to exclusion list)
18:08:37.46 -15:06:17.6 -- not an asteroid (will add it to exclusion list)
17:42:19.25 -18:03:02.9 -- not an asteroid (will add it to exclusion list)
17:42:51.28 -21:30:11.3 -- not an asteroid (will add it to exclusion list)
17:21:39.51 -20:32:06.4 -- not an asteroid (will add it to exclusion list)
18:09:01.00 -19:18:52.1 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
17:21:39.51 -20:32:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
17:32:49.11 -21:41:59.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:42:19.25 -18:03:02.9 -- does not seem to be a hot pixel (will add it to exclusion list)
17:42:51.28 -21:30:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
17:48:32.71 -21:06:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
17:51:18.15 -16:03:55.5 -- does not seem to be a hot pixel (will add it to exclusion list)
17:54:50.72 -21:37:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
17:55:40.90 -19:20:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
17:57:02.79 -19:20:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:01:11.67 -15:20:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:02:04.59 -15:03:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:05:28.56 -14:14:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
18:06:42.95 -14:19:09.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:08:20.91 -18:04:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:08:24.06 -15:03:29.5 -- does not seem to be a hot pixel (will add it to exclusion list)
18:08:37.46 -15:06:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
18:09:01.00 -19:18:52.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:09:24.82 -19:33:59.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:09:53.55 -14:36:26.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:10:04.85 -16:01:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
18:10:09.39 -16:12:28.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:10:40.34 -16:01:51.8 -- does not seem to be a hot pixel (will add it to exclusion list)
18:10:42.08 -15:27:27.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:10:51.68 -13:54:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:10:57.14 -14:29:13.3 -- does not seem to be a hot pixel (will add it to exclusion list)
18:11:26.78 -18:24:59.0 -- does not seem to be a hot pixel (will add it to exclusion list)
18:11:32.11 -14:28:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
18:11:38.21 -16:51:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
18:11:38.92 -15:26:11.0 -- 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)
17:21:39.51 -20:32:06.4 -- not a known variable star
17:32:49.11 -21:41:59.0 -- a known variable star
17:42:19.25 -18:03:02.9 -- not a known variable star
17:42:51.28 -21:30:11.3 -- a known variable star
17:48:32.71 -21:06:21.7 -- a known variable star
17:51:18.15 -16:03:55.5 -- not a known variable star
17:54:50.72 -21:37:11.0 -- a known variable star
17:55:40.90 -19:20:49.8 -- a known variable star
17:57:02.79 -19:20:16.3 -- a known variable star
18:01:11.67 -15:20:33.3 -- not a known variable star
18:02:04.59 -15:03:18.6 -- a known variable star
18:05:28.56 -14:14:20.7 -- not a known variable star
18:06:42.95 -14:19:09.5 -- not a known variable star
18:08:20.91 -18:04:34.2 -- a known variable star
18:08:24.06 -15:03:29.5 -- a known variable star
18:08:37.46 -15:06:17.6 -- a known variable star
18:09:01.00 -19:18:52.1 -- a known variable star
18:09:24.82 -19:33:59.0 -- a known variable star
18:09:53.55 -14:36:26.2 -- a known variable star
18:10:04.85 -16:01:42.4 -- not a known variable star
18:10:09.39 -16:12:28.8 -- not a known variable star
18:10:40.34 -16:01:51.8 -- a known variable star
18:10:42.08 -15:27:27.1 -- a known variable star
18:10:51.68 -13:54:18.0 -- not a known variable star
18:10:57.14 -14:29:13.3 -- not a known variable star
18:11:26.78 -18:24:59.0 -- a known variable star
18:11:32.11 -14:28:56.2 -- a known variable star
18:11:38.21 -16:51:28.1 -- not a known variable star
18:11:38.92 -15:26:11.0 -- a known variable star
Found 11 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
29 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
Adding identified Gaia sources from exclusion_list_gaiadr2.txt
Adding identified Gaia sources from exclusion_list_apass.txt
IS_THIS_TEST_RUN= NO ALLOW_EXCLUSION_LIST_UPDATE= YES
#### Adding the following to the exclusion list ####
17:21:39.51 -20:32:06.4
17:32:49.11 -21:41:59.0
17:42:19.25 -18:03:02.9
17:42:51.28 -21:30:11.3
17:48:32.71 -21:06:21.7
17:51:18.15 -16:03:55.5
17:54:50.72 -21:37:11.0
17:55:40.90 -19:20:49.8
17:57:02.79 -19:20:16.3
18:01:11.67 -15:20:33.3
18:02:04.59 -15:03:18.6
18:05:28.56 -14:14:20.7
18:06:42.95 -14:19:09.5
18:08:20.91 -18:04:34.2
18:08:24.06 -15:03:29.5
18:08:37.46 -15:06:17.6
18:09:01.00 -19:18:52.1
18:09:24.82 -19:33:59.0
18:09:53.55 -14:36:26.2
18:10:04.85 -16:01:42.4
18:10:09.39 -16:12:28.8
18:10:40.34 -16:01:51.8
18:10:42.08 -15:27:27.1
18:10:51.68 -13:54:18.0
18:10:57.14 -14:29:13.3
18:11:26.78 -18:24:59.0
18:11:32.11 -14:28:56.2
18:11:38.21 -16:51:28.1
18:11:38.92 -15:26:11.0
18:10:59.20 -13:38:31.3
18:11:33.23 -13:43:34.9
18:10:08.69 -15:18:42.4
18:08:35.90 -18:45:21.8
17:43:48.10 -16:26:49.5
18:00:11.85 -16:00:28.0
18:05:08.52 -14:30:31.4
18:07:31.15 -15:30:32.8
17:19:15.37 -20:49:54.3
18:10:17.67 -18:06:00.6
18:00:16.65 -16:16:25.5
17:37:42.59 -15:50:38.5
17:44:11.71 -20:16:56.9
18:11:18.67 -16:33:32.2
17:56:25.00 -22:01:30.4
17:43:00.04 -20:56:24.3
17:44:38.02 -13:45:48.8
18:10:59.18 -13:38:31.5
18:11:33.22 -13:43:34.9
18:11:02.57 -13:57:58.9
18:10:42.09 -13:48:36.1
17:19:03.15 -18:32:52.8
18:10:23.17 -13:36:41.1
18:10:41.52 -13:41:12.4
18:11:23.49 -13:47:54.0
18:11:13.28 -13:36:20.7
17:42:10.42 -15:43:15.7
18:04:40.89 -15:13:24.7
18:09:42.02 -13:42:13.9
17:35:39.04 -14:42:21.5
17:43:11.33 -15:00:38.7
18:04:28.39 -18:57:41.7
17:41:27.51 -14:27:39.7
17:37:39.74 -18:34:37.4
18:10:19.84 -15:50:01.5
18:10:27.18 -14:00:45.6
18:10:47.40 -14:25:15.4
####################################################
The observatory MPC code is V36
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461132.87662608 -observatory V36
23:05:24.71 -07:28:47.4 Mercury (0.4mag)
02:03:34.01 +12:08:05.3 Venus (-3.9mag)
23:38:58.67 -03:24:23.1 Mars (1.2mag)
07:07:28.59 +22:54:16.2 Jupiter (-2.2mag)
00:23:01.24 +00:10:10.8 Saturn (0.9mag)
03:45:00.50 +19:38:45.2 Uranus (5.8mag)
00:09:00.43 -00:27:00.3 Neptune (7.8mag)
20:32:59.22 -22:52:38.1 Pluto (14.5mag)
12:50:55.36 -09:37:51.7 Moon (-12.7mag)
-rw-r--r-- 1 apache apache 362 Apr 2 04:13 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461132.87662608:
07:07:36.62 +22:54:00.2 Io (5.7mag)
07:07:41.00 +22:53:52.0 Europa (5.8mag)
07:07:38.21 +22:53:50.4 Ganymede (5.3mag)
07:07:45.04 +22:53:35.3 Callisto (6.5mag)
07:11:18.33 +22:48:49.6 Himalia (15.3mag)
07:07:32.79 +22:54:08.1 Thebe (16.1mag)
07:11:10.37 +23:16:38.0 Elara (17.2mag)
07:05:25.92 +23:41:24.7 Pasiphae (17.3mag)
07:16:04.58 +22:50:42.2 Carme (18.4mag)
00:22:53.89 +00:10:35.8 Titan (8.8mag)
00:22:59.00 +00:10:18.3 Rhea (10.1mag)
00:23:10.51 +00:12:06.3 Iapetus (11.5mag)
00:22:51.63 +00:10:19.1 Hyperion (14.8mag)
00:24:48.06 +00:20:22.0 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Apr 2 04:14 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461132.87662608:
14:22:21.37 -04:37:23.7 JWST
19:46:21.12 +06:14:43.6 Chandra
08:34:20.92 -47:27:01.3 XMM-Newton
-rw-r--r-- 1 apache apache 96 Apr 2 04:14 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461132.87662608 -observatory V36
-> Warning: Longitude 255.61742 is outside valid range [-180, 180]
18:44:45.26 -28:02:28.2 14.0mag P/2010 H2 (Vales)
04:57:44.31 -70:20:53.7 17.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:29:59.26 +31:21:18.3 17.1mag C/2017 K2 (PANSTARRS)
17:30:52.75 +08:54:22.7 17.6mag C/2021 G2 (ATLAS)
23:06:05.69 +28:44:45.8 17.0mag C/2022 E2 (ATLAS)
04:13:44.37 +25:39:14.6 15.9mag C/2022 N2 (PANSTARRS)
09:01:34.82 +31:49:51.4 16.1mag C/2022 QE78 (ATLAS)
08:29:48.56 -01:40:29.3 17.2mag C/2022 R6 (PANSTARRS)
18:56:02.49 +17:21:49.2 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:44:23.97 -11:42:37.3 17.6mag P/2023 B1 (PANSTARRS)
09:15:14.68 -14:09:26.5 17.5mag C/2023 F3 (ATLAS)
21:38:47.65 +62:11:16.5 17.4mag C/2023 H5 (Lemmon)
19:28:32.25 -03:34:41.3 14.3mag C/2023 R1 (PANSTARRS)
21:42:54.91 +84:08:54.8 17.8mag C/2023 X2 (Lemmon)
06:13:57.71 +63:37:28.0 17.0mag C/2024 A1 (ATLAS)
04:41:37.51 +12:46:00.8 10.1mag C/2024 E1 (Wierzchos)
16:27:04.52 +04:09:08.3 17.4mag C/2024 G6 (ATLAS)
20:16:00.10 +11:43:10.8 14.8mag C/2024 J3 (ATLAS)
03:14:33.12 -24:32:44.8 16.4mag C/2024 T5 (ATLAS)
05:05:48.35 +48:53:27.7 17.6mag C/2025 J1 (Borisov)
14:33:46.66 +33:17:15.5 14.7mag C/2025 L1 (ATLAS)
03:04:54.98 -24:12:53.4 17.7mag C/2025 Q3 (ATLAS)
22:45:37.50 +19:45:17.5 10.7mag C/2025 R3 (PANSTARRS)
13:00:02.11 +02:08:24.7 17.5mag C/2025 Y1 (ATLAS)
01:20:42.23 +02:40:47.7 8.4mag C/2026 A1 (MAPS)
23:19:04.08 +34:22:05.1 14.1mag C/2026 B2 (Sun-Gao)
18:16:19.36 -10:23:30.5 12.6mag 10P/Tempel
15:17:08.76 +04:23:54.4 12.8mag 24P/Schaumasse
11:07:06.59 -02:00:19.3 15.7mag 29P/Schwassmann-Wachmann
17:54:20.82 -10:08:59.0 17.6mag 40P/Vaisala
10:39:55.24 -05:18:47.6 16.6mag 43P/Wolf-Harrington
01:27:42.94 +15:07:38.0 17.1mag 47P/Ashbrook-Jackson
06:46:59.73 +39:51:49.7 17.1mag 63P/Wild
23:11:12.97 -13:08:14.0 15.7mag 65P/Gunn
03:28:06.56 +16:17:20.3 15.8mag 76P/West-Kohoutek-Ikemura
00:35:50.25 +05:31:22.2 14.5mag 78P/Gehrels
22:20:15.93 -13:22:05.4 14.5mag 88P/Howell
01:32:54.07 +16:51:31.8 15.1mag 93P/Lovas
04:30:21.20 +31:29:31.6 16.3mag 123P/West-Hartley
08:14:37.63 +44:38:53.9 16.2mag 124P/Mrkos
02:12:29.37 +12:48:51.4 16.4mag 128P/Shoemaker-Holt
02:21:01.58 +12:44:52.5 17.4mag 131P/Mueller
00:17:10.37 +08:05:51.2 11.6mag 141P/Machholz
00:27:20.87 -00:11:49.6 11.6mag 141P-A/Machholz
23:20:13.22 -03:35:11.8 14.5mag 141P-D/Machholz
00:55:47.69 +01:23:40.2 18.0mag 141P-I/Machholz
00:24:35.79 -08:17:08.4 15.3mag 162P/SidingSpring
10:32:24.12 +31:42:29.7 17.7mag 164P/Christensen
06:11:30.35 +24:36:03.6 17.8mag 198P/ODAS
15:15:06.79 -01:41:18.0 17.2mag 210P/Christensen
20:56:20.93 -14:44:09.2 17.3mag 218P/LINEAR
17:10:11.78 -15:29:14.4 16.2mag 235P/LINEAR
05:05:48.27 +33:28:10.0 16.5mag 240P/NEAT
07:32:51.51 -06:45:16.4 17.6mag 242P/Spahr
15:46:53.20 +06:01:44.8 17.6mag 391P/Kowalski
07:29:56.48 +21:16:34.2 17.6mag 450P/LONEOS
05:16:43.46 +45:50:25.8 17.4mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.9K Apr 2 04:14 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
21:55:23.31 -34:48:53.90 ASASSN-26cj 2026-03-30.4 -1.47
11:19:50.70 -27:51:49.80 SN2026gvk 2026-03-30 15.48
11:53:57.02 -23:09:46.20 SN2026gzx 2026-03-28.75 15.27
07:13:46.14 -33:10:15.70 ASASSN-26ci 2026-03-28.15 15.14
09:03:36.09 -67:58:13.00 SN2026hkg 2026-03-28.19 15.82
07:03:00.72 +39:14:43.00 SN2026fin 2026-03-28.27 15.82
05:35:42.80 -63:44:05.50 ASASSN-26ch 2026-03-27.86 13.02
11:23:19.04 +34:22:38.00 SN2026fwt 2026-03-27.3 16.56
19:03:49.79 +37:04:05.20 ASASSN-26ce 2026-03-26.56 16.3
20:26:56.07 -52:54:06.50 AT2026hiy 2026-03-26.35 16.95
05:25:54.76 -30:15:35.80 ASASSN-26cg 2026-03-25.07 16.88
06:57:16.49 -26:54:37.20 SN2026fzb 2026-03-25.14 15.8
14:37:38.23 -43:00:52.30 ASASSN-26cd 2026-03-24.24 12.52
17:34:53.03 +06:04:29.70 AT2026gzl 2026-03-23.27 15.82
08:30:02.60 -35:12:47.50 ASASSN-26cf 2026-03-23.2 14.82
16:54:25.33 +37:49:56.60 SN 2026evz 2026-03-21.32 17.54
17:06:19.20 -18:54:19.50 ASASSN-26bx 2026-03-21.25 16.39
19:01:16.28 -29:29:23.10 ASASSN-26bw 2026-03-21.33 15.81
08:46:05.75 +10:47:39.80 ASASSN-26ca 2026-03-21.13 14.27
12:14:58.16 +63:47:16.20 SN 2026fvx 2026-03-21.12 15.6
18:02:55.90 -75:23:02.60 ASASSN-26bz 2026-03-21.32 16.16
12:16:02.88 -53:16:33.80 ASASSN-26cc 2026-03-20.04 15.48
13:08:21.85 +29:13:44.20 SN 2026fmh 2026-03-20.16 -0.33
19:56:38.48 -34:45:21.50 ASASSN-26cb 2026-03-20.35 -3.26
14:32:41.15 -41:38:48.50 ASASSN-26by 2026-03-20.15 -1.31
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.90 -45:55:38.40 ASASSN-26bt 2026-03-19.05 16.24
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 SDSS
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.89 -15:50:13.40 AT2026fdy 2026-03-10.5 16.39
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.33 -37:49:33.00 ASASSN-26bk 2026-03-2.06 13.58
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.29 +19:58:46.30 ASASSN-26be 2026-02-25.56 14.95
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
11:50:37.32 +55:21:13.70 SN 2026dix 2026-02-21.43 16.39
16:21:19.69 -63:47:29.40 ASASSN-26az 2026-02-21.03 17.02
02:45:30.93 -54:17:43.10 SN 2026cju 2026-02-21.04 17.54
01:58:40.68 +47:34:50.10 ASASSN-26av 2026-02-21.09 15.97
18:35:53.01 -42:31:38.90 ASASSN-26aw 2026-02-21.12 15.89
11:40:18.88 -39:45:09.20 ASASSN-26ax 2026-02-21.08 15.73
02:26:23.52 -51:42:29.80 ASASSN-26ay 2026-02-21.04 13.93
08:46:07.66 +01:17:43.90 ASASSN-26ba 2026-02-20.23 15.43
14:15:47.69 -48:05:16.40 SN2026dez 2026-02-19.19 15.93
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.22 -11:25:16.10 AT2026bzh 2026-02-12.16 17.22
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
06:26:33.34 -54:06:39.90 AT2026cih 2026-02-8.06 17.26
23:08:59.40 -88:59:11.60 SN 2026bsu 2026-02-8.03 16.02
01:04:14.94 -62:31:02.30 SN 2026azk 2026-02-8.04 16.41
08:44:55.41 +64:55:09.90 SN 2026anq 2026-02-7.16 17.62
12:37:42.99 +33:26:05.40 SN 2026bnm 2026-02-7.29 16.74
-rw-r--r-- 1 apache apache 5.8K Apr 2 04:13 asassn_transients_list.txt
############################################################
Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
22:34:01.26 +39:53:32.8 TCP J22340126+3953328 2026-01-17.5738 16.79Cmag
00:42:52.36 +41:16:13.3 PNV J00425236+4116133 2026-01-18.5502 17.41Cmag
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
09:55:38.83 +69:05:21.7 PNV J09553883+6905217 2026-04-01.893 19.4mag
-rw-r--r-- 1 apache apache 187K Apr 2 04:13 tocp_transients_list.txt
############################################################
Truncated list of recent TNS transients from https://www.wis-tns.org/ :
08:08:11.420 -04:49:30.53 AT 2026hkf 2026-03-14.22 21.0121
04:20:57.978 -04:44:24.49 AT 2026hke 2026-03-26.13 19.8012
08:08:20.226 -14:40:00.64 AT 2026hkd 2026-03-07.19 20.1897
07:59:24.647 +57:00:58.39 AT 2026hkc 2026-03-14.20 20.9477
13:58:50.252 -17:03:03.26 AT 2026hkb 2026-03-23.24 19.315
08:55:52.185 -18:24:10.01 AT 2026hka 2026-03-20.39 19.87
19:49:11.846 -17:41:20.03 AT 2026hjz 2026-03-24.76 19.09
17:23:18.071 +42:30:08.80 AT 2026hjy 2026-03-15.19 19.329
15:36:56.914 -04:11:42.38 AT 2026hjx 2026-03-25.78 20.01
16:12:19.428 -02:04:41.40 AT 2026hjw 2026-03-24.64 20.22
11:18:56.464 -28:36:26.32 AT 2026hjv 2026-03-21.92 19.08
13:33:46.392 +11:46:20.90 AT 2026hju 2026-03-20.24 18.89
11:08:39.309 -42:07:08.38 AT 2026hjt 2026-03-25.18 19.306
18:40:00.884 -46:00:21.86 AT 2026hjs 2026-03-22.37 19.141
10:49:28.071 -32:24:01.15 AT 2026hjr 2026-03-21.92 19.476
08:13:57.386 +50:00:46.26 AT 2026hjq 2026-03-08.96 20.035
18:55:05.624 -41:25:59.25 AT 2026hjp 2026-03-24.79 20.17
14:10:06.186 +10:00:51.42 AT 2026hjo 2026-03-24.40 20.2791
08:47:29.260 +16:55:56.97 AT 2026hjn 2026-03-20.25 20.8588
08:53:19.672 -26:00:27.80 AT 2026hjm 2026-03-26.19 19.4129
-rw-r--r-- 1 apache apache 29K Apr 2 04:13 tns_transients_list.txt
