This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461136.9219,11.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260406.4219 11.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4179590872275212032,2461136.9219,13.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4179590872275212032 20260406.4219 13.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V6494 Sgr,2461136.9219,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V6494 Sgr 20260406.4219 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461136.9219,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 20260406.4219 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.9219,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260406.4219 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.9219,13.39,0.05,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
target 20260406.4219 13.39CV 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
V0984 Sgr,2461136.9219,10.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V0984 Sgr 20260406.4219 10.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
TW Sgr,2461136.9219,10.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
TW Sgr 20260406.4219 10.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J194931-1740.8,2461136.9219,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J194931-1740.8 20260406.4219 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461118.99455619 19.03.2026 11:51:59.655 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
First image: 2461118.99455619 19.03.2026 11:51:59.655 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Last image: 2461136.92227486 06.04.2026 10:07:54.548 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 6
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.53
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: 5 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): 9701
Objects passed selection criteria: 9697
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 9168.75
Average stars matched: 8571.5 (93.486 %)
Memory usage VmPeak: 115876 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 6 05:15:28 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: 2461118.99455619 19.03.2026 11:51:59.655 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
First image: 2461118.99455619 19.03.2026 11:51:59.655 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Last image: 2461136.92227486 06.04.2026 10:07:54.548 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 137
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.17
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: 58 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): 98458
Objects passed selection criteria: 98306
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 92354.5
Average stars matched: 82840.5 (89.6984 %)
Memory usage VmPeak: 1883104 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 6 05:17:43 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-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits
SExtractor catalog cache: saved Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat to cache
SExtractor catalog cache: saved Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.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-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.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: 2461136.92157439
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'
Plate-solving the images
'tns_transients_list.txt' -> '../tns_transients_list.txt'
wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits exists and is non-empty
Saving wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits to local_wcs_cache/
'wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits' -> 'local_wcs_cache/wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits'
wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits exists and is non-empty
Saving wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits to local_wcs_cache/
'wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits' -> 'local_wcs_cache/wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits'
wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits exists and is non-empty
Saving wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits to local_wcs_cache/
'wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits' -> 'local_wcs_cache/wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits'
wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits exists and is non-empty
Saving wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits to local_wcs_cache/
'wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits' -> 'local_wcs_cache/wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits'
The image scale is 5.88"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 19:33:22.678 -18:00:40.27
Second-epoch image center 19:33:21.166 -18:00:12.10
Angular distance between the image centers 0.0099 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 19:33:22.678 -18:00:40.27
Second-epoch image center 19:33:18.377 -18:00:17.13
Angular distance between the image centers 0.0182 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 19:33:21.166 -18:00:12.10
Second-epoch second image center 19:33:18.377 -18:00:17.13
Angular distance between the image centers 0.01114 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-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits &> /tmp/tmp.QDHPZ1Qd9S
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits &> /tmp/tmp.4ZQquHnCW3
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits &> /tmp/tmp.hHL4tjPjG4
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits &> /tmp/tmp.IbJzupE7Cd
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits
Calibrating the magnitude scale
Found non-empty wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.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-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.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-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
Found non-empty wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
The reference image (wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits) and catalog (wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat) found
'wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat' -> 'wcsmag.cat'
Read 11017 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 284.7685 to 301.7245 deg, Dec -23.3021 to -12.5136 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 284.7685 to 301.7245 deg, Dec -23.3021 to -12.5136 deg
Loaded 13778 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): 8233 out of 8546 total matches.
Matched with Tycho-2 8546 out of 11017 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.784657
a=0.000000 b=1.000000 c=22.784657
From vast_summary.log: estimated ref. image limiting mag.: -8.53
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.25
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.25
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.5 pix Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
2.0 pix Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
2.5 pix fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits
2.5 pix fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits
Limiting magnitude estimates:
14.3 mag. Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
14.6 mag. Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
14.0 mag. fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits
14.0 mag. fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 11.3 (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.QDHPZ1Qd9S (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.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-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits' -> 'wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
WCS_IMAGE_NAME=wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
WCS-calibrated image found: wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Checking if the catalog wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits alredy exist and is non-empty...
Catalog wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
WCS catalog name: wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=800, passed=11017
Got 11017 stars (including 10207 good ones) from the SExtractor catalog wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
util/solve_plate_with_UCAC5 got 11017 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.1'
Seting catalog search parameters based on the expected field of view 938.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013029 (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 0.010423 (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 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 937 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 961 matched stars entering correct_measured_positions(), 10657 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 10657 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
WARNING: Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 10656 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 959 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits -region wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.4ZQquHnCW3 (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-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.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_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.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-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.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-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits' -> 'wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
WCS_IMAGE_NAME=wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
WCS-calibrated image found: wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
Checking if the catalog wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits alredy exist and is non-empty...
Catalog wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
WCS catalog name: wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1081, passed=13469
Got 13469 stars (including 12369 good ones) from the SExtractor catalog wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat
util/solve_plate_with_UCAC5 got 13469 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (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 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 933 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 13041 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 13040 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
WARNING: Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 13040 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 959 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits -region wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.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.hHL4tjPjG4 (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_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.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_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits
WCS-calibrated image found: wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits
Checking if the catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits
WCS catalog name: wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=618, passed=8809
Got 8809 stars (including 8184 good ones) from the SExtractor catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits.cat
util/solve_plate_with_UCAC5 got 8809 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.4'
Seting catalog search parameters based on the expected field of view 938.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013033 (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 0.010427 (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 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 929 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 8541 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
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 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 8541 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
WARNING: Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 8541 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
Excluding outliers - 953 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits -region wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.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.IbJzupE7Cd (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_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.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_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits
WCS-calibrated image found: wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits
Checking if the catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits
WCS catalog name: wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=622, passed=8812
Got 8812 stars (including 8179 good ones) from the SExtractor catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits.cat
util/solve_plate_with_UCAC5 got 8812 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.3'
Seting catalog search parameters based on the expected field of view 938.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013032 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010426 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 931 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 8555 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
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 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 8555 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
WARNING: Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 8555 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
Excluding outliers - 951 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits -region wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.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-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits'
Saving fully-calibrated image wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits'
Saving fully-calibrated image wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits'
Saving fully-calibrated image wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits'
Preparing the HTML report for the field Sgr-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out22329.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out22332.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out22333.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out22315.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22315_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
Preparing report for the candidate 22315_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
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Considering the candidate 22320_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 22320_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:16:31.55 -18:01:36.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 22329_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 22329_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:19:06.48 -15:53:18.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.29, MAG_FAINT_SEARCH_LIMIT=12.27)GAIADR2_OUTPUT=# 2.144 4183978645232402048 289.77647789453 -15.88812432953 11.0282 10.2125 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.144#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22332_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 22332_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:39:16.06 -14:14:55.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.51, MAG_FAINT_SEARCH_LIMIT=12.49)GAIADR2_OUTPUT=# 0.919 4182974103913299200 294.81669891096 -14.24868956014 11.0155 10.0295 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.919#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22333_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 22333_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:29:19.18 -15:11:44.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.43, MAG_FAINT_SEARCH_LIMIT=12.41)GAIADR2_OUTPUT=# 1.144 4181531128043505152 292.32963413644 -15.19558650718 12.3203 10.4147 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.144#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 7s
Prepared the HTML report for the field Sgr-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
19:12:14.22 -19:18:41.7
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-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits
SExtractor catalog cache: saved Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat to cache
SExtractor catalog cache: saved Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.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-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Creating symlink local_wcs_cache/wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
Creating symlink local_wcs_cache/wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits
Creating symlink local_wcs_cache/wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.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-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits exists and is non-empty
wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits exists and is non-empty
wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits exists and is non-empty
wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits exists and is non-empty
The image scale is 5.88"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 19:33:22.678 -18:00:40.27
Second-epoch image center 19:33:21.166 -18:00:12.10
Angular distance between the image centers 0.0099 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 19:33:22.678 -18:00:40.27
Second-epoch image center 19:33:18.377 -18:00:17.13
Angular distance between the image centers 0.0182 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 19:33:21.166 -18:00:12.10
Second-epoch second image center 19:33:18.377 -18:00:17.13
Angular distance between the image centers 0.01114 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-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits &> /tmp/tmp.NhlBjcD524
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits &> /tmp/tmp.USXaJHfodQ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits &> /tmp/tmp.7ilF232Kgm
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits &> /tmp/tmp.g6hKu0AtS3
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits
Calibrating the magnitude scale
Found non-empty wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.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-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.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-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
Found non-empty wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
The reference image (wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits) and catalog (wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat) found
'wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat' -> 'wcsmag.cat'
Read 101850 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 284.7602 to 301.7245 deg, Dec -23.3064 to -12.5129 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 284.7602 to 301.7245 deg, Dec -23.3064 to -12.5129 deg
Loaded 13790 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): 10156 out of 11996 total matches.
Matched with Tycho-2 11996 out of 101850 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.547522
a=0.000000 b=1.000000 c=22.547522
From vast_summary.log: estimated ref. image limiting mag.: -8.17
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.38
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.38
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 97 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.4 pix Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
2.0 pix Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
2.4 pix fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits
2.3 pix fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits
Limiting magnitude estimates:
14.4 mag. Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
14.7 mag. Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
14.2 mag. fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits
14.2 mag. fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits
All-image limiting magnitude estimate: 14.2 (SNR ) 13.5 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.NhlBjcD524 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.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-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits' -> 'wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
WCS_IMAGE_NAME=wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
WCS-calibrated image found: wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Checking if the catalog wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits alredy exist and is non-empty...
Catalog wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
WCS catalog name: wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=8404, passed=101839
Got 101839 stars (including 93311 good ones) from the SExtractor catalog wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat
util/solve_plate_with_UCAC5 got 101839 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.1'
Seting catalog search parameters based on the expected field of view 938.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013029 (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 0.010423 (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 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 930 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 98878 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 98875 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
WARNING: Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 98875 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 958 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits -region wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.USXaJHfodQ (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-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.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_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.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-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.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-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits' -> 'wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
WCS_IMAGE_NAME=wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
WCS-calibrated image found: wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
Checking if the catalog wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits alredy exist and is non-empty...
Catalog wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat corresponding to the image wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
WCS catalog name: wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=12676, passed=138124
Got 138124 stars (including 125221 good ones) from the SExtractor catalog wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat
util/solve_plate_with_UCAC5 got 138124 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.0'
Seting catalog search parameters based on the expected field of view 942.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013083 (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 0.010467 (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 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 134051 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
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 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 134050 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
WARNING: Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 134051 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits -region wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.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.7ilF232Kgm (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_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.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_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits
WCS-calibrated image found: wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits
Checking if the catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits
WCS catalog name: wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=5845, passed=82204
Got 82204 stars (including 76277 good ones) from the SExtractor catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits.cat
util/solve_plate_with_UCAC5 got 82204 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.4'
Seting catalog search parameters based on the expected field of view 938.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013033 (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 0.010427 (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 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 925 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 79857 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
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 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 79857 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
WARNING: Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 79848 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits -region wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.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.g6hKu0AtS3 (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_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.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_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits
WCS-calibrated image found: wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits
Checking if the catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits.cat corresponding to the image wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits
WCS catalog name: wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=6107, passed=84075
Got 84075 stars (including 77874 good ones) from the SExtractor catalog wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits.cat
util/solve_plate_with_UCAC5 got 84075 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.3'
Seting catalog search parameters based on the expected field of view 938.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013032 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010426 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 927 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 81823 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
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 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 81820 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
WARNING: Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 81814 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Excluding outliers - 955 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits -region wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.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-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/wcs_Sgr-03-Q2b1x1_2026-03-19_06-51-59_20.00sec_-15.00C_LIGHT_0232.fits
Saving fully-calibrated image wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.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_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/wcs_Sgr-03-Q2b1x1_2026-03-22_06-39-42_20.00sec_-15.00C_LIGHT_0390.fits
Saving fully-calibrated image wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.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_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-06-54_20.00sec_-4.90C_LIGHT_0411.fits
Saving fully-calibrated image wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.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_2026-04-06_CI_Sgr-03-Q2b1x1_050840_TTUQ2b1x1_31726_53Akw4Yp/wcs_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412.fits
Preparing the HTML report for the field Sgr-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out124611.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148177.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148183.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148185.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148192.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148195.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148196.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148198.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148199.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148203.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148205.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148207.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148208.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148213.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148220.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148222.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148223.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148228.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148229.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148231.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148237.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148239.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148244.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148254.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148373.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148450.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148521.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148530.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148539.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148562.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148583.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148590.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148607.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148629.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148635.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148666.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148671.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148676.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148697.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148707.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148731.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148739.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148754.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148762.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148803.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148830.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148854.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148887.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148904.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148915.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148924.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148943.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out148980.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out12226.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out148174.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out148249.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out148451.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out148748.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out148797.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out15661.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out54430.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 20s
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: 5s
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Considering the candidate 148174_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
Preparing report for the candidate 148174_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
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Considering the candidate 148177_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148177_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:21:38.62 -14:45:49.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 2.863 4184715008782833920 290.41009581634 -14.76385547495 13.7259 12.9825 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.863#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148183_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148183_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:19:34.96 -16:43:28.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 3.034 4183853713221291392 289.89484159679 -16.72420710729 13.3266 12.5409 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.034#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148185_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148185_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:26:21.54 -16:51:19.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)
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Considering the candidate 148192_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148192_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:28:21.61 -15:32:29.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 2.335 4181377780529866368 292.08936852321 -15.54159417209 13.5276 12.9590 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.335#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148195_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148195_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:34:10.81 -14:27:17.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 1.823 4183061274571260800 293.54454138058 -14.45457446252 13.3481 12.7963 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.823#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148196_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148196_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:15:25.96 -15:17:27.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 0.890 4184262216156056064 288.85818014567 -15.29130254325 13.7195 12.9628 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.890#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148198_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148198_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:21:51.27 -16:44:27.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 1.138 4180857715833952128 290.46354599982 -16.74058200019 13.8327 13.3537 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.138#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148199_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148199_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:12:39.71 -17:54:10.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 0.939 4087600644263568128 288.16529477046 -17.90309825065 13.4545 12.7404 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.939#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148203_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148203_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:18:59.02 -14:51:43.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 1.967 4184379172398551168 289.74598509927 -14.86273686358 13.3806 12.6469 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.967#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148205_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148205_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:07:19.60 -16:46:02.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 0.407 4088710979215514880 286.83163550086 -16.76714104793 13.7387 13.1844 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.407#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148207_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148207_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:06:53.06 -16:23:35.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 2.033 4088786364483338112 286.72050116719 -16.39319329246 13.4524 12.8884 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.033#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148208_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148208_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:09:14.01 -14:56:35.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 2.969 4089192767152340480 287.30789232059 -14.94256992284 13.4096 12.7039 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.969#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148209_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148209_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:15:38.25 -14:00:07.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148211_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148211_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:22:52.67 -18:00:30.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148213_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148213_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:23:09.44 -17:08:43.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)
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Considering the candidate 148220_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148220_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:38:03.04 -13:53:09.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 3.720 4183187026910912896 294.51161535551 -13.88613471062 13.4030 12.7260 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.720#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148222_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148222_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:09:00.53 -18:31:13.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 3.180 4087180871341990272 287.25299939862 -18.51983914024 13.3029 12.4008 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.180#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148223_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148223_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:15:49.82 -18:49:24.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 2.856 4084108354814976000 288.95704593213 -18.82289123471 13.2636 12.7997 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.856#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148228_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148228_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:11:23.32 -14:42:06.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.50, MAG_FAINT_SEARCH_LIMIT=14.48)
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Considering the candidate 148229_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148229_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:06:59.07 -15:52:08.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 1.035 4088843156819172224 286.74600952298 -15.86881818410 13.2379 12.5769 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.035#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148231_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148231_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:30:22.28 -16:47:15.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)
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Considering the candidate 148233_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148233_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
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Considering the candidate 148237_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148237_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:04:34.44 -19:12:30.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)
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Considering the candidate 148239_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148239_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:04:44.02 -20:57:15.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 0.744 4082259663455408256 286.18328769572 -20.95436252563 12.4832 11.3051 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.744#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148242_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148242_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:12:28.71 -15:21:45.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148244_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148244_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:14:05.94 -20:17:27.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)
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Considering the candidate 148246_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148246_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:10:25.55 -15:39:56.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148247_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148247_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:22:52.23 -14:52:56.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148249_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
Preparing report for the candidate 148249_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
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Considering the candidate 148254_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148254_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:15:37.74 -17:28:41.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 0.831 4087724781692043776 288.90716626126 -17.47846644143 11.8116 11.0644 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.831#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148256_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148256_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:15:59.11 -14:26:46.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148302_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148302_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:12:14.22 -19:18:41.9 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 148334_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148334_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:17:43.06 -18:55:29.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 148373_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148373_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:05:15.88 -16:52:49.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 1.052 4088343982854916352 286.31594118886 -16.88069702944 11.9566 11.4795 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.052#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148435_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148435_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:08:52.34 -18:57:25.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148450_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148450_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:14:01.56 -14:01:08.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)GAIADR2_OUTPUT=# 3.355 4185433054287821568 288.50566891855 -14.01847709247 12.1825 11.4521 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.355#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148451_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
Preparing report for the candidate 148451_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
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Considering the candidate 148462_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148462_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:17:36.66 -15:57:04.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148466_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148466_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:04:37.42 -21:46:01.4 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 148485_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148485_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:18:07.52 -18:52:41.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148519_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148519_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:36:26.35 -18:52:32.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 148521_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148521_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:11:15.49 -20:42:02.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 2.189 4082147822501784832 287.81389285739 -20.70081519659 12.5229 11.8262 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.189#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148530_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148530_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:21:47.81 -16:04:59.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 1.851 4183992384817749504 290.44867323437 -16.08329818434 12.3486 11.5877 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.851#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148539_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148539_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:11:56.79 -14:41:19.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 2.612 4185287613832366464 287.98587501396 -14.68874386823 12.6994 11.8896 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.612#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148546_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148546_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:34:17.90 -16:20:39.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148549_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148549_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:29:33.00 -21:19:26.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148562_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148562_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:10:36.00 -16:57:41.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 0.593 4087919536999532416 287.64986384663 -16.96151731934 12.8529 12.1295 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.593#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148568_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148568_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:26:21.68 -21:14:45.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148574_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148574_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:24:45.06 -18:37:40.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148583_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148583_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:13:01.09 -20:12:16.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 2.729 4083673085647159424 288.25377014587 -20.20491935872 12.4718 11.4516 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.729#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148586_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148586_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:16:35.34 -14:57:31.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148589_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148589_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:10:00.08 -17:29:53.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148590_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148590_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:28:51.38 -16:07:08.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 1.835 4181133345349009792 292.21377916656 -16.11849885093 12.6964 11.9461 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.835#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148596_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148596_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:09:51.27 -20:04:04.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148607_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148607_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:18:12.23 -17:24:07.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 1.158 4084735694916482816 289.55063625065 -17.40190518006 12.6717 11.9240 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.158#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148629_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148629_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:06:28.55 -15:19:17.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 1.942 4089153356536476160 286.61840166332 -15.32160861200 12.9531 12.3805 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.942#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148635_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148635_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:38:20.04 -14:55:12.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.92, MAG_FAINT_SEARCH_LIMIT=13.90)GAIADR2_OUTPUT=# 4.188 4182864290188878592 294.58361774454 -14.92121335511 13.1098 12.5360 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.188#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148666_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148666_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:25:01.76 -20:43:29.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.92, MAG_FAINT_SEARCH_LIMIT=13.90)GAIADR2_OUTPUT=# 1.944 6773226995610709888 291.25676006932 -20.72489853200 12.9146 12.4128 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.944#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148667_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148667_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:09:02.04 -17:06:29.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148671_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148671_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:05:18.00 -16:06:50.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)
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Considering the candidate 148676_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148676_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:19:40.69 -22:11:53.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 3.128 6772645319601580160 289.91862585960 -22.19838370818 12.7742 12.0858 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.128#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148697_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148697_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:18:13.56 -17:24:08.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 1.479 4084735690612323072 289.55647549398 -17.40268805398 13.2071 12.4133 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.479#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148707_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148707_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:17:56.51 -14:40:17.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 0.742 4184398005841192576 289.48525377546 -14.67161359489 13.1658 12.3417 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.742#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148715_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148715_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:15:21.71 -17:15:35.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148731_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148731_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:17:35.51 -15:58:08.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 3.173 4184161301602476928 289.39711904291 -15.96864534090 13.1264 12.3527 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.173#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148734_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148734_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:26:42.84 -16:47:38.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148739_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148739_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:12:09.81 -15:48:34.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 1.848 4088891608359033344 288.04052450815 -15.80919624938 13.1166 12.3305 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.848#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148748_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
Preparing report for the candidate 148748_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
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Considering the candidate 148751_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148751_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:19:31.21 -21:10:14.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148754_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148754_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:14:49.88 -14:08:28.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 2.324 4185240163031639808 288.70732609905 -14.14172369089 13.3314 12.6019 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.324#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148762_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148762_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:34:17.75 -16:24:11.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 3.865 4180403514446819200 293.57346711942 -16.40413130107 13.3750 12.7158 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.865#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148780_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148780_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:05:40.36 -18:17:33.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148786_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148786_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:26:05.66 -15:02:43.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 148788_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148788_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:14:07.82 -18:04:15.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148793_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148793_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:08:11.62 -16:38:31.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148795_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148795_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:11:57.52 -20:13:43.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148797_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
Preparing report for the candidate 148797_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
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Considering the candidate 148803_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148803_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:17:41.21 -17:21:40.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 3.953 4084725249555682944 289.42075981682 -17.36071203031 11.5580 10.0667 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.953#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148819_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148819_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:06:46.43 -17:27:49.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148830_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148830_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:26:20.97 -15:11:34.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 1.691 4184452118117745152 291.58697999048 -15.19264206476 13.3332 12.7897 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.691#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148854_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148854_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:29:38.54 -15:21:48.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 2.098 4181473373621490176 292.41069149377 -15.36396231740 13.4830 12.7599 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.098#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148866_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148866_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:30:03.23 -19:22:56.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148887_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148887_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:16:12.37 -18:31:30.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)
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Considering the candidate 148904_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148904_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:04:39.98 -15:07:14.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 3.412 4089127591049909632 286.16586833474 -15.11996176647 14.0579 12.2620 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.412#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148915_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148915_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:37:15.81 -13:58:25.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 2.221 4183179746947792000 294.31527490584 -13.97381476555 13.3831 12.7772 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.221#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148924_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148924_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:09:39.50 -17:24:30.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 3.542 4087878717629293824 287.41355374343 -17.40860696262 13.6056 13.0402 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.542#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148943_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148943_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:20:04.30 -14:13:00.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 1.367 4184793756995752576 290.01752919744 -14.21672186172 12.4962 11.0771 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.367#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 148952_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148952_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:10:19.70 -17:45:21.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 148980_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 148980_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:21:37.10 -17:19:20.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 2.911 4180756109780338688 290.40402108792 -17.32183953636 13.4656 11.3721 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.911#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 15661_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
Preparing report for the candidate 15661_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
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Considering the candidate 12226_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
Preparing report for the candidate 12226_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
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Considering the candidate 48852_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 48852_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:16:31.61 -18:01:36.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 124611_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 124611_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:37:52.16 -14:08:14.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)
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Considering the candidate 54430_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
Preparing report for the candidate 54430_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
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Considering the candidate 112656_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 112656_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
**** FOUND 19:26:18.53 -19:10:22.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 116964_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412
The candidate 116964_fd_Sgr-03-Q2b1x1_2026-04-06_05-07-54_20.00sec_-4.90C_LIGHT_0412 did not pass the final checks
