This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq
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
V7343 Sgr,2461132.9096,9.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V7343 Sgr 20260402.4096 9.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4077983216147590400,2461132.9096,12.26,0.05,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 4077983216147590400 20260402.4096 12.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
OGLE-BLG-LPV-195890,2461132.9096,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
OGLE-BLG-LPV-195890 20260402.4096 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
OGLE-BLG-ELL-019360,2461132.9096,11.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
OGLE-BLG-ELL-019360 20260402.4096 11.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1955 Sgr,2461132.9096,12.45,0.05,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
V1955 Sgr 20260402.4096 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
V1864 Sgr,2461132.9096,11.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1864 Sgr 20260402.4096 11.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
LO Sgr,2461132.9096,11.39,0.05,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
LO Sgr 20260402.4096 11.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461118.98182816 19.03.2026 11:33:39.953 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
First image: 2461118.98182816 19.03.2026 11:33:39.953 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
Last image: 2461132.91079362 02.04.2026 09:51:22.569 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.61
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 13479
Objects passed selection criteria: 13451
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 10693.8
Average stars matched: 10407.8 (97.3255 %)
Memory usage VmPeak: 119408 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 1 15:05:04 CDT 2026
VaST build number 1.0rc88-372-gf0c1109d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-01)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 2 04:53:30 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: 2461118.98182816 19.03.2026 11:33:39.953 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
First image: 2461118.98182816 19.03.2026 11:33:39.953 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
Last image: 2461132.91079362 02.04.2026 09:51:22.569 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 53
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.27
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: 43 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): 163896
Objects passed selection criteria: 163575
Measurements per detected object (mean, median, min, max): 2.9 3.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 3.0 2 4
Average stars detected per image: 129082
Average stars matched: 122355 (94.788 %)
Memory usage VmPeak: 1932360 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 1 15:05:04 CDT 2026
VaST build number 1.0rc88-372-gf0c1109d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-01)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 2 04:57:01 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-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits
SExtractor catalog cache: saved Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits.cat to cache
SExtractor catalog cache: saved Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.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-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461132.90840593
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits exists and is non-empty
Saving wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits to local_wcs_cache/
'wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits' -> 'local_wcs_cache/wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits'
wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits exists and is non-empty
Saving wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits to local_wcs_cache/
'wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits' -> 'local_wcs_cache/wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits'
wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits exists and is non-empty
Saving wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits to local_wcs_cache/
'wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits' -> 'local_wcs_cache/wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits'
wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits exists and is non-empty
Saving wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits to local_wcs_cache/
'wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits' -> 'local_wcs_cache/wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.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 18:14:25.391 -25:59:48.34
Second-epoch image center 18:14:37.840 -25:59:01.61
Angular distance between the image centers 0.05 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 18:14:25.391 -25:59:48.34
Second-epoch image center 18:14:35.006 -25:59:47.17
Angular distance between the image centers 0.04 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 18:14:37.840 -25:59:01.61
Second-epoch second image center 18:14:35.006 -25:59:47.17
Angular distance between the image centers 0.01652 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-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits &> /tmp/tmp.2NINDtgFqd
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits &> /tmp/tmp.Wz3ZtIRVmI
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits &> /tmp/tmp.3TATpz54BU
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits &> /tmp/tmp.DjsI0UOLC9
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits
Calibrating the magnitude scale
Found non-empty wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.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-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits and wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.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-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits and wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits.cat
Found non-empty wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits and wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits.cat
The reference image (wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits) and catalog (wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits.cat) found
'wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits.cat' -> 'wcsmag.cat'
Read 16719 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 264.4302 to 282.6069 deg, Dec -31.2746 to -20.4260 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 264.4302 to 282.6069 deg, Dec -31.2746 to -20.4260 deg
Loaded 19370 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): 11077 out of 11719 total matches.
Matched with Tycho-2 11719 out of 16719 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.803743
a=0.000000 b=1.000000 c=22.803743
From vast_summary.log: estimated ref. image limiting mag.: -8.61
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.19
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.19
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.4 pix Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
2.4 pix Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits
2.9 pix fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits
3.2 pix fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits
Limiting magnitude estimates:
14.2 mag. Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
14.2 mag. Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits
13.2 mag. fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits
13.5 mag. fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits
All-image limiting magnitude estimate: 13.2 (SNR ) 10.7 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.2NINDtgFqd (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_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.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-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits' -> 'wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
WCS_IMAGE_NAME=wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
WCS-calibrated image found: wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
Checking if the catalog wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits.cat corresponding to the image wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits alredy exist and is non-empty...
Catalog wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits.cat corresponding to the image wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
WCS catalog name: wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1482, passed=16719
Got 16719 stars (including 15219 good ones) from the SExtractor catalog wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits.cat
util/solve_plate_with_UCAC5 got 16719 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.71"
Removing outliers...
Correcting the measured astrometric positions...
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 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.69"
Estimated accuracy of the plate solution: 0.83"
Excluding outliers - 916 stars left (next iteration limit 1008)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits -region wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.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.Wz3ZtIRVmI (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_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.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-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits' -> 'wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits
WCS_IMAGE_NAME=wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits
WCS-calibrated image found: wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits
Checking if the catalog wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits.cat corresponding to the image wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits alredy exist and is non-empty...
Catalog wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits.cat corresponding to the image wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits
WCS catalog name: wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1517, passed=16501
Got 16501 stars (including 14968 good ones) from the SExtractor catalog wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits.cat
util/solve_plate_with_UCAC5 got 16501 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.69"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.65"
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 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.65"
Estimated accuracy of the plate solution: 0.81"
Excluding outliers - 917 stars left (next iteration limit 1007)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits -region wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.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.3TATpz54BU (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits
WCS-calibrated image found: wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits
Checking if the catalog wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits.cat corresponding to the image wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits.cat corresponding to the image wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits
WCS catalog name: wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=639, passed=6935
Got 6935 stars (including 6294 good ones) from the SExtractor catalog wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits.cat
util/solve_plate_with_UCAC5 got 6935 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 293 to 350 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.87"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.85"
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 293 to 350 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.86"
Estimated accuracy of the plate solution: 0.92"
Excluding outliers - 914 stars left (next iteration limit 1005)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits -region wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.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.DjsI0UOLC9 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits
WCS-calibrated image found: wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits
Checking if the catalog wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits.cat corresponding to the image wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits.cat corresponding to the image wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits
WCS catalog name: wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=664, passed=8637
Got 8637 stars (including 7968 good ones) from the SExtractor catalog wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits.cat
util/solve_plate_with_UCAC5 got 8637 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 922 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 1.15"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 1.17"
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 293 to 349 (Dec -31.3 to -20.5)
Done reading UCAC5 zone files...
Matched 923 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 1.18"
Estimated accuracy of the plate solution: 1.29"
Excluding outliers - 901 stars left (next iteration limit 994)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits -region wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.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-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits'
Saving fully-calibrated image wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits'
Saving fully-calibrated image wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits'
Saving fully-calibrated image wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits'
Preparing the HTML report for the field Sgr-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out20984.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 4s
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 20984_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 20984_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 5s
Prepared the HTML report for the field Sgr-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
18:36:23.71 -23:54:07.3
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-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits
SExtractor catalog cache: saved Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits.cat to cache
SExtractor catalog cache: saved Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.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-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
Creating symlink local_wcs_cache/wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits
Creating symlink local_wcs_cache/wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits
Creating symlink local_wcs_cache/wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.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-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits exists and is non-empty
wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits exists and is non-empty
wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits exists and is non-empty
wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.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 18:14:25.391 -25:59:48.34
Second-epoch image center 18:14:37.840 -25:59:01.61
Angular distance between the image centers 0.05 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 18:14:25.391 -25:59:48.34
Second-epoch image center 18:14:35.006 -25:59:47.17
Angular distance between the image centers 0.04 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 18:14:37.840 -25:59:01.61
Second-epoch second image center 18:14:35.006 -25:59:47.17
Angular distance between the image centers 0.01652 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-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits &> /tmp/tmp.cXgB84tfb3
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits &> /tmp/tmp.CQm2eiSemR
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits &> /tmp/tmp.QMw3QmmPJC
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits &> /tmp/tmp.ZqLVhmjkfZ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits
Calibrating the magnitude scale
Found non-empty wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.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-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits and wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.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-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits and wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits.cat
Found non-empty wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits and wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits.cat
The reference image (wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits) and catalog (wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits.cat) found
'wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits.cat' -> 'wcsmag.cat'
Read 200125 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 264.4217 to 282.6069 deg, Dec -31.2857 to -20.4094 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 264.4217 to 282.6069 deg, Dec -31.2857 to -20.4094 deg
Loaded 19419 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): 12665 out of 16837 total matches.
Matched with Tycho-2 16837 out of 200125 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.519710
a=0.000000 b=1.000000 c=22.519710
From vast_summary.log: estimated ref. image limiting mag.: -8.27
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 34 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
2.2 pix Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits
2.5 pix fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits
2.9 pix fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits
Limiting magnitude estimates:
14.2 mag. Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
14.3 mag. Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits
13.3 mag. fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits
13.6 mag. fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits
All-image limiting magnitude estimate: 13.3 (SNR ) 12.6 (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.cXgB84tfb3 (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_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.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-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits' -> 'wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
WCS_IMAGE_NAME=wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
WCS-calibrated image found: wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
Checking if the catalog wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits.cat corresponding to the image wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits alredy exist and is non-empty...
Catalog wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits.cat corresponding to the image wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
WCS catalog name: wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits.cat
SExtractor catalog parsing summary: zero_flux=4, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=27, blended=25986, passed=200094
Got 200094 stars (including 173914 good ones) from the SExtractor catalog wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits.cat
util/solve_plate_with_UCAC5 got 200094 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.63"
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 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.63"
Estimated accuracy of the plate solution: 0.74"
Excluding outliers - 924 stars left (next iteration limit 1015)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits -region wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.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.CQm2eiSemR (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_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.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-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits' -> 'wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits
WCS_IMAGE_NAME=wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits
WCS-calibrated image found: wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits
Checking if the catalog wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits.cat corresponding to the image wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits alredy exist and is non-empty...
Catalog wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits.cat corresponding to the image wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits
WCS catalog name: wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=27, blended=27503, passed=207780
Got 207780 stars (including 180064 good ones) from the SExtractor catalog wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits.cat
util/solve_plate_with_UCAC5 got 207780 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.64"
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 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.64"
Estimated accuracy of the plate solution: 0.72"
Excluding outliers - 926 stars left (next iteration limit 1016)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits -region wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.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.QMw3QmmPJC (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits
WCS-calibrated image found: wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits
Checking if the catalog wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits.cat corresponding to the image wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits.cat corresponding to the image wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits
WCS catalog name: wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=6888, passed=85546
Got 85546 stars (including 78567 good ones) from the SExtractor catalog wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits.cat
util/solve_plate_with_UCAC5 got 85546 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 293 to 350 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.81"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.78"
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 293 to 350 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.78"
Estimated accuracy of the plate solution: 0.90"
Excluding outliers - 920 stars left (next iteration limit 1010)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits -region wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.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.ZqLVhmjkfZ (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits
WCS-calibrated image found: wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits
Checking if the catalog wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits.cat corresponding to the image wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits.cat corresponding to the image wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits
WCS catalog name: wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=8173, passed=82707
Got 82707 stars (including 74484 good ones) from the SExtractor catalog wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits.cat
util/solve_plate_with_UCAC5 got 82707 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010418 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 925 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 1.08"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 1.06"
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 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 925 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 1.06"
Estimated accuracy of the plate solution: 1.18"
Excluding outliers - 908 stars left (next iteration limit 1002)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits -region wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.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-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/wcs_Sgr-04-Q2b1x1_2026-03-19_06-33-39_20.00sec_-14.90C_LIGHT_0219.fits
Saving fully-calibrated image wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/wcs_Sgr-04-Q2b1x1_2026-03-19_06-34-52_20.00sec_-14.90C_LIGHT_0220.fits
Saving fully-calibrated image wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-47-56_20.00sec_-14.90C_LIGHT_0066.fits
Saving fully-calibrated image wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sgr-04-Q2b1x1_045200_TTUQ2b1x1_14832_pKeZo1oq/wcs_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067.fits
Preparing the HTML report for the field Sgr-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out234721.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234728.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234780.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234787.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234812.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234824.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234837.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out234840.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out234784.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234791.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out234818.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out74872.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out74954.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out88828.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 10s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 4s
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Considering the candidate 234715_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067
The candidate 234715_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 18:34:01.17 -22:27:56.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234721_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067
The candidate 234721_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 18:37:23.20 -21:32:39.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)
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Considering the candidate 234728_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067
The candidate 234728_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 18:28:04.38 -24:06:23.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)
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Considering the candidate 234748_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067
The candidate 234748_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 18:29:00.90 -25:01:52.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234780_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067
The candidate 234780_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 18:18:27.78 -27:45:15.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.35, MAG_FAINT_SEARCH_LIMIT=13.33)
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Considering the candidate 234784_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 234784_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 234787_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067
The candidate 234787_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 18:02:52.97 -26:55:02.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)
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Considering the candidate 234791_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 234791_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 234805_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067
The candidate 234805_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 234806_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067
The candidate 234806_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 17:47:18.63 -26:41:41.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234812_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067
The candidate 234812_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 18:20:46.75 -30:10:25.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.05, MAG_FAINT_SEARCH_LIMIT=13.03)GAIADR2_OUTPUT=# 4.009 4049480228222925184 275.19421289944 -30.17460596790 11.7845 10.7570 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.009#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234818_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 234818_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 234824_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067
The candidate 234824_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 17:57:47.04 -26:53:14.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.14, MAG_FAINT_SEARCH_LIMIT=13.12)GAIADR2_OUTPUT=# 3.795 4063634825519564800 269.44717941138 -26.88718113020 12.2524 11.3726 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.795#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234837_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067
The candidate 234837_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 17:48:46.84 -21:52:45.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.64, MAG_FAINT_SEARCH_LIMIT=12.62)GAIADR2_OUTPUT=# 0.701 4118543959567528704 267.19509782796 -21.87898265224 11.1906 10.3022 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.701#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234840_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067
The candidate 234840_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 17:54:06.83 -27:30:14.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.55, MAG_FAINT_SEARCH_LIMIT=12.53)GAIADR2_OUTPUT=# 1.992 4063509245055524480 268.52793851516 -27.50358275232 11.1821 10.2459 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.992#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 234992_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067
The candidate 234992_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 18:20:49.38 -29:48:14.6 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 235004_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067
The candidate 235004_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
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Considering the candidate 235023_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067
The candidate 235023_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 18:03:28.98 -24:23:01.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235170_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067
The candidate 235170_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 18:14:24.83 -21:42:59.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 235192_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067
The candidate 235192_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 235346_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067
The candidate 235346_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 18:28:05.92 -26:44:09.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 235633_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067
The candidate 235633_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 18:07:26.08 -22:05:59.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235655_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067
The candidate 235655_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 18:24:30.14 -29:31:14.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235710_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067
The candidate 235710_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 18:18:34.04 -25:36:32.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 235715_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067
The candidate 235715_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 18:28:09.72 -26:46:52.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 235928_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067
The candidate 235928_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 18:16:19.44 -30:12:52.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 235948_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067
The candidate 235948_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 18:10:30.05 -27:54:07.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 97022_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067
The candidate 97022_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 18:20:54.78 -26:33:49.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 74954_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 74954_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 86981_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067
The candidate 86981_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 18:12:00.04 -27:00:07.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 112586_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067
The candidate 112586_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks
**** FOUND 18:28:29.86 -25:47:51.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 74872_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067
Preparing report for the candidate 74872_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067
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Considering the candidate 26293_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067
The candidate 26293_fd_Sgr-04-Q2b1x1_2026-04-02_04-51-22_20.00sec_-15.00C_LIGHT_0067 did not pass the final checks