This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 08 03.1179 2461255.6179 9.38 18:50:01.08 -23:33:28.5
11.58235 -10.20620 galactic Sgr Second-epoch detections are separated by 0.4" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.8 Flora 1 -0 1 9.6 -0 -0
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits at 18:50:01.08 -23:33:28.5: 14.32 +/- 99.00 upperlimit
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits at 18:50:01.08 -23:33:28.5: 14.73 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461255.6179,9.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260803.1179 9.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1179 2461255.6179 11.43 18:47:50.41 -28:31:01.0
6.79089 -11.85406 galactic Sgr Second-epoch detections are separated by 0.5" and 6.0 pix
The object was found in VSX22" Gaia DR3 4071502209177016832
Type: E
# Max. Min./Amp. JD0 Period
17.670 G 17.850 G 0.265482000000
NOTE: the measured brightness disagrees with the variable-star record above, but is consistent with the asteroid identification below - so this is likely the asteroid rather than an outburst of the variable.
The object was found in astcheck.128 Nemesis 1 -0 1 11.7 0 -0
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits at 18:47:50.41 -28:31:01.0: 14.30 +/- 99.00 upperlimit
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits at 18:47:50.41 -28:31:01.0: 14.73 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4071502209177016832,2461255.6179,11.43,0.05,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 4071502209177016832 20260803.1179 11.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 03.1179 2461255.6179 12.89 19:23:02.36 -22:38:44.3
15.62591 -16.76614 galactic Sgr Second-epoch detections are separated by 1.3" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.182 Elsa 1 1 1 12.7 -0 -0
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits at 19:23:02.36 -22:38:44.3: 14.54 +/- 99.00 upperlimit
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits at 19:23:02.36 -22:38:44.3: 15.03 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461255.6179,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260803.1179 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461147.90695453 17.04.2026 09:45:50.871 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits
First image: 2461147.90695453 17.04.2026 09:45:50.871 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits
Last image: 2461255.61818633 03.08.2026 02:50:01.299 /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.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.: -8.36
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: 3
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
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 5683
Objects passed selection criteria: 5681
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 6020.25
Average stars matched: 5090.75 (84.5604 %)
Memory usage VmPeak: 233280 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 29 18:03:05 CDT 2026
VaST build number 1.0rc89-187-gf9db235a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-29)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Aug 2 21:53:35 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: 2461147.90695453 17.04.2026 09:45:50.871 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits
First image: 2461147.90695453 17.04.2026 09:45:50.871 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits
Last image: 2461255.61818633 03.08.2026 02:50:01.299 /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 118
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.01
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: 45 seconds
Number of parallel threads: 3
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
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 81988
Objects passed selection criteria: 81824
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 79786.8
Average stars matched: 70610.5 (88.499 %)
Memory usage VmPeak: 582784 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 29 18:03:05 CDT 2026
VaST build number 1.0rc89-187-gf9db235a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-29)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Aug 2 21:55:14 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 --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits
SExtractor catalog cache: saved Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits.cat to cache
SExtractor catalog cache: saved Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.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-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.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: 2461255.61769226
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-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits exists and is non-empty
Saving wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits to local_wcs_cache/
'wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits' -> 'local_wcs_cache/wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits'
wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits exists and is non-empty
Saving wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits to local_wcs_cache/
'wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits' -> 'local_wcs_cache/wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits'
wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits exists and is non-empty
Saving wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits to local_wcs_cache/
'wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits' -> 'local_wcs_cache/wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits'
wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits exists and is non-empty
Saving wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits to local_wcs_cache/
'wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits' -> 'local_wcs_cache/wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits (1st reference image)
verification OK: wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits
Image size: 942.3'x627.3' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 19:11:51.170 -26:00:19.21 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits (1st new image)
verification OK: wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits
Image size: 937.7'x624.6' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 19:12:01.369 -25:59:44.38 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 19:11:51.170 -26:00:19.21
Second-epoch image center 19:12:01.369 -25:59:44.38
Angular distance between the image centers 0.0394 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits (2nd new image)
verification OK: wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits
Image size: 937.7'x624.6' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 19:12:04.069 -25:59:42.87 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 19:11:51.170 -26:00:19.21
Second-epoch image center 19:12:04.069 -25:59:42.87
Angular distance between the image centers 0.0493 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 19:12:01.369 -25:59:44.38
Second-epoch second image center 19:12:04.069 -25:59:42.87
Angular distance between the image centers 0.01012 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits &> /tmp/tmp.D6xzfEKUpm
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits &> /tmp/tmp.NaVAHk4ZFf
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits &> /tmp/tmp.RouooG4Dad
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits &> /tmp/tmp.ANErjZgvHz
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits
Calibrating the magnitude scale
Found non-empty wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.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-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits and wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
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-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits and wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits.wcscat
Found non-empty wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits and wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits.wcscat
The reference image (wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits) and catalog (wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits.wcscat) found
'wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits.wcscat' -> 'wcsmag.cat'
Read 6297 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 278.5158 to 296.7476 deg, Dec -31.5070 to -20.1279 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 278.5158 to 296.7476 deg, Dec -31.5070 to -20.1279 deg
Loaded 14496 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): 5080 out of 5188 total matches.
Matched with Tycho-2 5188 out of 6297 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.136550
a=0.000000 b=1.000000 c=22.136550
From vast_summary.log: estimated ref. image limiting mag.: -8.36
Updating vast_summary.log: Estimated ref. image limiting mag.: 13.78
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 13.78
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 6297 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 278.5158 to 296.7476 deg, Dec -31.5070 to -20.1279 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 278.5158 to 296.7476 deg, Dec -31.5070 to -20.1279 deg
Loaded 14496 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): 5080 out of 5188 total matches.
Matched with Tycho-2 5188 out of 6297 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits
Forced-photometry filter: calibrated wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits -> calib.txt_param_ref_wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits (aperture=6.0)
Read 10687 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 278.9550 to 297.0903 deg, Dec -31.2648 to -20.5647 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 278.9550 to 297.0903 deg, Dec -31.2648 to -20.5647 deg
Loaded 13345 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): 7818 out of 8091 total matches.
Matched with Tycho-2 8091 out of 10687 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits
Forced-photometry filter: calibrated wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits -> calib.txt_param_ref_wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits (aperture=6.1)
____ 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: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits
2.3 pix Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits
2.2 pix fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits
2.3 pix fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits
Limiting magnitude estimates:
13.8 mag. Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits
14.1 mag. Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits
13.7 mag. fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits
13.7 mag. fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits
All-image limiting magnitude estimate: 13.7 (SNR ) 10.8 (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 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.D6xzfEKUpm (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.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-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits' -> 'wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits
WCS_IMAGE_NAME=wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits
WCS-calibrated image found: wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits
Checking if the catalog wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits.wcscat corresponding to the image wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits alredy exist and is non-empty...
Catalog wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits.wcscat corresponding to the image wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits
WCS catalog name: wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=388, bad_region=879, passed=6297
Got 6297 stars (including 5071 good ones) from the SExtractor catalog wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits.wcscat
util/solve_plate_with_UCAC5 got 6297 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010470 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.5 to -20.1)
Done reading UCAC5 zone files...
Matched 4925 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4821 matched stars entering correct_measured_positions(), 4823 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4821 matched stars entering correct_measured_positions(), 5599 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.5 to -20.1)
Done reading UCAC5 zone files...
Matched 4924 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4821 matched stars entering correct_measured_positions(), 5599 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 4821 matched stars entering correct_measured_positions(), 5599 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 4821 stars left (next iteration limit 5303)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits N_match=4821 sigma_overall_arcsec=0.464 sigma_q1_arcsec=0.459 sigma_q2_arcsec=0.392 sigma_q3_arcsec=0.513 sigma_q4_arcsec=0.378 n_q1=1652 n_q2=620 n_q3=1756 n_q4=793 worst_quadrant_to_overall_ratio=1.106
The image catalog is written to wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits -region wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.NaVAHk4ZFf (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_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.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-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits' -> 'wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits
WCS_IMAGE_NAME=wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits
WCS-calibrated image found: wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits
Checking if the catalog wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits.wcscat corresponding to the image wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits alredy exist and is non-empty...
Catalog wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits.wcscat corresponding to the image wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits
WCS catalog name: wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=726, bad_region=1847, passed=10687
Got 10687 stars (including 8208 good ones) from the SExtractor catalog wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits.wcscat
util/solve_plate_with_UCAC5 got 10687 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.6)
Done reading UCAC5 zone files...
Matched 4913 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4820 matched stars entering correct_measured_positions(), 4822 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4820 matched stars entering correct_measured_positions(), 9226 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.6)
Done reading UCAC5 zone files...
Matched 4914 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4821 matched stars entering correct_measured_positions(), 9226 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Accuracy estimation diagnostic: 4820 matched stars entering correct_measured_positions(), 9226 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Excluding outliers - 4820 stars left (next iteration limit 5302)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits N_match=4820 sigma_overall_arcsec=0.563 sigma_q1_arcsec=0.561 sigma_q2_arcsec=0.470 sigma_q3_arcsec=0.627 sigma_q4_arcsec=0.488 n_q1=1636 n_q2=777 n_q3=1508 n_q4=899 worst_quadrant_to_overall_ratio=1.114
The image catalog is written to wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits -region wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.RouooG4Dad (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_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.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_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits
WCS-calibrated image found: wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits
Checking if the catalog wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits.wcscat corresponding to the image wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits.wcscat corresponding to the image wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits
WCS catalog name: wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=514, bad_region=1060, passed=5987
Got 5987 stars (including 4485 good ones) from the SExtractor catalog wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits.wcscat
util/solve_plate_with_UCAC5 got 5987 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.6)
Done reading UCAC5 zone files...
Matched 4416 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4332 matched stars entering correct_measured_positions(), 4334 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4332 matched stars entering correct_measured_positions(), 5141 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.6)
Done reading UCAC5 zone files...
Matched 4416 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4334 matched stars entering correct_measured_positions(), 5141 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.65"
Accuracy estimation diagnostic: 4334 matched stars entering correct_measured_positions(), 5141 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.66"
Excluding outliers - 4334 stars left (next iteration limit 4765)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4334 robust_rms=6.943 arcsec worst_quadrant_rms=9.327 arcsec
SIP_REFIT: SIP order 3 trial: matched=4334 robust_rms=0.705 arcsec worst_quadrant_rms=0.837 arcsec
SIP_REFIT: SIP order 5 trial: matched=4334 robust_rms=0.584 arcsec worst_quadrant_rms=0.671 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4334 robust_rms_before=0.953 arcsec robust_rms_before_corrected=0.658 arcsec robust_rms_after=0.584 arcsec worst_quadrant_rms_before=0.731 worst_quadrant_rms_after=0.671
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.731 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits N_match=4334 sigma_overall_arcsec=0.662 sigma_q1_arcsec=0.685 sigma_q2_arcsec=0.586 sigma_q3_arcsec=0.760 sigma_q4_arcsec=0.543 n_q1=1465 n_q2=677 n_q3=1415 n_q4=777 worst_quadrant_to_overall_ratio=1.148
The image catalog is written to wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits -region wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.ANErjZgvHz (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_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.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_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits
WCS-calibrated image found: wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits
Checking if the catalog wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits.wcscat corresponding to the image wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits.wcscat corresponding to the image wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits
WCS catalog name: wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=565, bad_region=1098, passed=6201
Got 6201 stars (including 4641 good ones) from the SExtractor catalog wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits.wcscat
util/solve_plate_with_UCAC5 got 6201 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.6)
Done reading UCAC5 zone files...
Matched 4572 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4485 matched stars entering correct_measured_positions(), 4487 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4485 matched stars entering correct_measured_positions(), 5331 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.6)
Done reading UCAC5 zone files...
Matched 4570 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4484 matched stars entering correct_measured_positions(), 5331 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.61"
Accuracy estimation diagnostic: 4484 matched stars entering correct_measured_positions(), 5331 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Excluding outliers - 4484 stars left (next iteration limit 4933)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4484 robust_rms=6.837 arcsec worst_quadrant_rms=9.503 arcsec
SIP_REFIT: SIP order 3 trial: matched=4484 robust_rms=0.694 arcsec worst_quadrant_rms=0.826 arcsec
SIP_REFIT: SIP order 5 trial: matched=4484 robust_rms=0.564 arcsec worst_quadrant_rms=0.657 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4484 robust_rms_before=0.952 arcsec robust_rms_before_corrected=0.612 arcsec robust_rms_after=0.564 arcsec worst_quadrant_rms_before=0.740 worst_quadrant_rms_after=0.657
verification OK: wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits
verification OK: wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits
Image size: 937.8'x624.7' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 19:12:04.045 -25:59:43.50 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 6201 stars ###
'wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/correct_sextractor_wcs_catalog_usingxy2sky124108.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 0.952 -> 0.564 arcsec)
WCS_QUALITY_DIAG: file=fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits N_match=4484 sigma_overall_arcsec=0.616 sigma_q1_arcsec=0.579 sigma_q2_arcsec=0.669 sigma_q3_arcsec=0.732 sigma_q4_arcsec=0.498 n_q1=1541 n_q2=701 n_q3=1448 n_q4=794 worst_quadrant_to_overall_ratio=1.187
The image catalog is written to wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits -region wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits sigma_overall=0.464 worst_q_ratio=1.106
ref2=Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits sigma_overall=0.563 worst_q_ratio=1.114
new1=fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits sigma_overall=0.662 worst_q_ratio=1.148
new2=fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits sigma_overall=0.616 worst_q_ratio=1.187
reference average sigma_overall=0.5135 worst_q_ratio=1.11
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284_astrometric_residuals.png (4821 matched stars from wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.44 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055_astrometric_residuals.png (4820 matched stars from wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.51 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014_astrometric_residuals.png (4334 matched stars from wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.62 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015_astrometric_residuals.png (4484 matched stars from wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.48 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits'
Saving fully-calibrated image wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits'
Preparing the HTML report for the field Sgr-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits at 18:50:01.08 -23:33:28.5: 14.32 +/- 99.00 upperlimit
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits at 18:50:01.08 -23:33:28.5: 14.73 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out23692.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
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 23692_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
Preparing report for the candidate 23692_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 8s
Prepared the HTML report for the field Sgr-05-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 ####
18:50:01.08 -23:33:28.5
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits
SExtractor catalog cache: saved Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits.cat to cache
SExtractor catalog cache: saved Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.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-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits
Creating symlink local_wcs_cache/wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits
Creating symlink local_wcs_cache/wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits
Creating symlink local_wcs_cache/wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.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-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits exists and is non-empty
wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits exists and is non-empty
wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits exists and is non-empty
wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits (1st reference image)
verification OK: wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits
Image size: 942.3'x627.3' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 19:11:51.170 -26:00:19.21 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits (1st new image)
verification OK: wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits
Image size: 937.7'x624.6' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 19:12:01.369 -25:59:44.38 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 19:11:51.170 -26:00:19.21
Second-epoch image center 19:12:01.369 -25:59:44.38
Angular distance between the image centers 0.0394 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits (2nd new image)
verification OK: wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits
Image size: 937.7'x624.6' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 19:12:04.069 -25:59:42.87 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 19:11:51.170 -26:00:19.21
Second-epoch image center 19:12:04.069 -25:59:42.87
Angular distance between the image centers 0.0493 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 19:12:01.369 -25:59:44.38
Second-epoch second image center 19:12:04.069 -25:59:42.87
Angular distance between the image centers 0.01012 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits &> /tmp/tmp.eG3p2ak0nk
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits &> /tmp/tmp.D1UfctEWNP
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits &> /tmp/tmp.yPB9Mvdag2
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits &> /tmp/tmp.TkxkO6JiUs
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits
Calibrating the magnitude scale
Found non-empty wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.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-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits and wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
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-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits and wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits.wcscat
Found non-empty wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits and wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits.wcscat
The reference image (wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits) and catalog (wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits.wcscat) found
'wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits.wcscat' -> 'wcsmag.cat'
Read 84103 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 278.4864 to 296.7493 deg, Dec -31.5437 to -20.0386 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 278.4864 to 296.7493 deg, Dec -31.5437 to -20.0386 deg
Loaded 14698 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): 10647 out of 11707 total matches.
Matched with Tycho-2 11707 out of 84103 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 21.872800
a=0.000000 b=1.000000 c=21.872800
From vast_summary.log: estimated ref. image limiting mag.: -8.01
Updating vast_summary.log: Estimated ref. image limiting mag.: 13.86
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 13.86
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 84103 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 278.4864 to 296.7493 deg, Dec -31.5437 to -20.0386 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 278.4864 to 296.7493 deg, Dec -31.5437 to -20.0386 deg
Loaded 14698 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): 10647 out of 11707 total matches.
Matched with Tycho-2 11707 out of 84103 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits
Forced-photometry filter: calibrated wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits -> calib.txt_param_ref_wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits (aperture=4.4)
Read 118893 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 278.9116 to 297.0918 deg, Dec -31.2648 to -20.5524 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 278.9116 to 297.0918 deg, Dec -31.2648 to -20.5524 deg
Loaded 13402 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): 10008 out of 11606 total matches.
Matched with Tycho-2 11606 out of 118893 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits
Forced-photometry filter: calibrated wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits -> calib.txt_param_ref_wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits (aperture=4.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 71 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits
2.1 pix Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits
2.0 pix fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits
2.0 pix fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits
Limiting magnitude estimates:
13.9 mag. Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits
14.3 mag. Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits
13.8 mag. fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits
13.8 mag. fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 13.2 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.eG3p2ak0nk (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.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-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits' -> 'wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits
WCS_IMAGE_NAME=wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits
WCS-calibrated image found: wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits
Checking if the catalog wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits.wcscat corresponding to the image wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits alredy exist and is non-empty...
Catalog wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits.wcscat corresponding to the image wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits
WCS catalog name: wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=4218, bad_region=8669, passed=84096
Got 84096 stars (including 71322 good ones) from the SExtractor catalog wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits.wcscat
util/solve_plate_with_UCAC5 got 84096 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010470 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.5 to -20.0)
Done reading UCAC5 zone files...
Matched 4917 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4821 matched stars entering correct_measured_positions(), 4822 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4821 matched stars entering correct_measured_positions(), 77554 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.5 to -20.0)
Done reading UCAC5 zone files...
Matched 4918 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4823 matched stars entering correct_measured_positions(), 77554 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 4823 matched stars entering correct_measured_positions(), 77554 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 4823 stars left (next iteration limit 5303)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits N_match=4823 sigma_overall_arcsec=0.434 sigma_q1_arcsec=0.419 sigma_q2_arcsec=0.391 sigma_q3_arcsec=0.497 sigma_q4_arcsec=0.363 n_q1=1678 n_q2=686 n_q3=1639 n_q4=820 worst_quadrant_to_overall_ratio=1.145
The image catalog is written to wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits -region wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.D1UfctEWNP (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_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.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-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits' -> 'wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits
WCS_IMAGE_NAME=wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits
WCS-calibrated image found: wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits
Checking if the catalog wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits.wcscat corresponding to the image wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits alredy exist and is non-empty...
Catalog wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits.wcscat corresponding to the image wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits
WCS catalog name: wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=8799, bad_region=12630, passed=118884
Got 118884 stars (including 98108 good ones) from the SExtractor catalog wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits.wcscat
util/solve_plate_with_UCAC5 got 118884 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.6)
Done reading UCAC5 zone files...
Matched 4918 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4835 matched stars entering correct_measured_positions(), 4836 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4835 matched stars entering correct_measured_positions(), 109622 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.6)
Done reading UCAC5 zone files...
Matched 4920 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4834 matched stars entering correct_measured_positions(), 109622 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 4834 matched stars entering correct_measured_positions(), 109622 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 4834 stars left (next iteration limit 5318)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits N_match=4834 sigma_overall_arcsec=0.551 sigma_q1_arcsec=0.553 sigma_q2_arcsec=0.509 sigma_q3_arcsec=0.625 sigma_q4_arcsec=0.499 n_q1=1702 n_q2=791 n_q3=1422 n_q4=919 worst_quadrant_to_overall_ratio=1.135
The image catalog is written to wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits -region wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.yPB9Mvdag2 (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_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.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_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits
WCS-calibrated image found: wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits
Checking if the catalog wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits.wcscat corresponding to the image wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits.wcscat corresponding to the image wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits
WCS catalog name: wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=4217, bad_region=9194, passed=78913
Got 78913 stars (including 65768 good ones) from the SExtractor catalog wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits.wcscat
util/solve_plate_with_UCAC5 got 78913 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.6)
Done reading UCAC5 zone files...
Matched 4922 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4832 matched stars entering correct_measured_positions(), 4837 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4832 matched stars entering correct_measured_positions(), 72139 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.6)
Done reading UCAC5 zone files...
Matched 4921 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4833 matched stars entering correct_measured_positions(), 72139 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Accuracy estimation diagnostic: 4833 matched stars entering correct_measured_positions(), 72139 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Excluding outliers - 4833 stars left (next iteration limit 5315)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits N_match=4833 sigma_overall_arcsec=0.627 sigma_q1_arcsec=0.605 sigma_q2_arcsec=0.587 sigma_q3_arcsec=0.783 sigma_q4_arcsec=0.532 n_q1=1734 n_q2=820 n_q3=1370 n_q4=909 worst_quadrant_to_overall_ratio=1.250
The image catalog is written to wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits -region wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.TkxkO6JiUs (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_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.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_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits
WCS_IMAGE_NAME=wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits
WCS-calibrated image found: wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits
Checking if the catalog wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits.wcscat corresponding to the image wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits alredy exist and is non-empty...
Catalog wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits.wcscat corresponding to the image wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits
WCS catalog name: wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=3, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=4464, bad_region=9368, passed=79549
Got 79549 stars (including 66032 good ones) from the SExtractor catalog wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits.wcscat
util/solve_plate_with_UCAC5 got 79549 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.6)
Done reading UCAC5 zone files...
Matched 4918 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4833 matched stars entering correct_measured_positions(), 4834 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4833 matched stars entering correct_measured_positions(), 72701 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.6)
Done reading UCAC5 zone files...
Matched 4918 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4833 matched stars entering correct_measured_positions(), 72701 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Accuracy estimation diagnostic: 4833 matched stars entering correct_measured_positions(), 72701 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.60"
Excluding outliers - 4833 stars left (next iteration limit 5316)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits N_match=4833 sigma_overall_arcsec=0.604 sigma_q1_arcsec=0.607 sigma_q2_arcsec=0.549 sigma_q3_arcsec=0.760 sigma_q4_arcsec=0.495 n_q1=1739 n_q2=822 n_q3=1363 n_q4=909 worst_quadrant_to_overall_ratio=1.259
The image catalog is written to wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits -region wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.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_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-49-18_20.00sec_-0.00C_LIGHT_0014.fits
Saving fully-calibrated image wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.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_2026-08-02_CI_Sgr-05-Q2b1x1_215107_TTUQ2b1x1_4168059_duripcwf/wcs_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015.fits
Preparing the HTML report for the field Sgr-05-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits at 19:14:40.92 -22:35:28.3: 13.38 +/- 0.12 detection
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits at 18:47:28.87 -29:19:58.5: 13.26 +/- 0.16 detection
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits at 19:12:15.43 -25:27:58.9: 13.78 +/- 0.16 detection
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits at 18:57:03.46 -30:12:31.2: 13.34 +/- 0.14 detection
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits at 18:54:10.19 -23:55:00.2: 13.61 +/- 0.18 detection
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits at 19:26:43.97 -22:38:54.1: 13.64 +/- 0.16 detection
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits at 19:03:20.45 -29:16:25.7: 13.11 +/- 0.11 detection
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits at 18:42:30.24 -28:31:37.7: 13.49 +/- 0.20 detection
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits at 19:12:15.43 -25:27:58.9: 13.63 +/- 0.10 detection
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits at 18:57:03.46 -30:12:31.2: 13.24 +/- 0.09 detection
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits at 19:26:43.97 -22:38:54.1: 13.54 +/- 0.09 detection
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits at 18:54:10.19 -23:55:00.2: 13.38 +/- 0.10 detection
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits at 19:14:40.92 -22:35:28.3: 13.48 +/- 0.08 detection
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits at 18:47:28.87 -29:19:58.5: 13.25 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.67 +/- 0.08
Forced photometry reference-image weighted average: 13.26 +/- 0.07
Forced photometry reference-image weighted average: 13.57 +/- 0.08
Forced photometry reference-image weighted average: 13.43 +/- 0.09
Forced photometry reference-image weighted average: 13.45 +/- 0.07
Forced photometry filter REJECTED candidate at 19:12:15.43 -25:27:58.9: ref_mag=13.67 +/- 0.08 new_mean_mag=13.3186 delta=0.35 (need > 0.90)
Forced photometry filter REJECTED candidate at 18:57:03.46 -30:12:31.2: ref_mag=13.26 +/- 0.07 new_mean_mag=13.4079 delta=-0.14 (need > 0.90)
Forced photometry filter REJECTED candidate at 19:26:43.97 -22:38:54.1: ref_mag=13.57 +/- 0.08 new_mean_mag=13.4385 delta=0.13 (need > 0.90)
Forced photometry filter REJECTED candidate at 18:54:10.19 -23:55:00.2: ref_mag=13.43 +/- 0.09 new_mean_mag=13.4053 delta=0.03 (need > 0.90)
Forced photometry reference-image weighted average: 13.26 +/- 0.08
Forced photometry filter REJECTED candidate at 19:14:40.92 -22:35:28.3: ref_mag=13.45 +/- 0.07 new_mean_mag=13.4712 delta=-0.02 (need > 0.90)
Forced photometry filter REJECTED candidate at 18:47:28.87 -29:19:58.5: ref_mag=13.26 +/- 0.08 new_mean_mag=13.1348 delta=0.12 (need > 0.90)
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits at 19:03:20.45 -29:16:25.7: 12.97 +/- 0.06 detection
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits at 18:45:45.36 -29:07:02.3: 13.12 +/- 0.13 detection
Forced photometry reference-image weighted average: 13.01 +/- 0.05
Forced photometry filter REJECTED candidate at 19:03:20.45 -29:16:25.7: ref_mag=13.01 +/- 0.05 new_mean_mag=13.3328 delta=-0.32 (need > 0.90)
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits at 18:42:30.24 -28:31:37.7: 13.17 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.23 +/- 0.09
Forced photometry filter REJECTED candidate at 18:42:30.24 -28:31:37.7: ref_mag=13.23 +/- 0.09 new_mean_mag=13.1507 delta=0.08 (need > 0.90)
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits at 18:45:37.85 -27:22:02.5: 12.75 +/- 0.09 detection
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits at 18:45:45.36 -29:07:02.3: 13.19 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.17 +/- 0.08
Forced photometry filter REJECTED candidate at 18:45:45.36 -29:07:02.3: ref_mag=13.17 +/- 0.08 new_mean_mag=13.0522 delta=0.11 (need > 0.90)
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits at 18:46:48.59 -28:57:34.2: 12.84 +/- 0.10 detection
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits at 18:45:00.55 -28:19:16.0: 12.73 +/- 0.10 detection
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits at 19:30:23.03 -25:09:59.1: 13.01 +/- 0.09 detection
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits at 19:26:02.51 -27:13:10.6: 12.45 +/- 0.06 detection
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits at 18:51:19.81 -25:36:57.9: 12.65 +/- 0.07 detection
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits at 18:42:14.56 -27:42:14.2: 12.95 +/- 0.12 detection
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits at 18:45:37.85 -27:22:02.5: 12.69 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.05
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits at 19:04:40.74 -26:32:27.8: 12.59 +/- 0.06 detection
Forced photometry filter REJECTED candidate at 18:45:37.85 -27:22:02.5: ref_mag=12.71 +/- 0.05 new_mean_mag=12.9097 delta=-0.20 (need > 0.90)
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits at 18:45:00.55 -28:19:16.0: 12.79 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.77 +/- 0.05
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits at 18:46:48.59 -28:57:34.2: 12.87 +/- 0.07 detection
Forced photometry filter REJECTED candidate at 18:45:00.55 -28:19:16.0: ref_mag=12.77 +/- 0.05 new_mean_mag=12.7384 delta=0.03 (need > 0.90)
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits at 19:30:23.03 -25:09:59.1: 12.75 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.86 +/- 0.06
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits at 18:51:19.81 -25:36:57.9: 12.83 +/- 0.06 detection
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits at 18:42:14.56 -27:42:14.2: 12.93 +/- 0.07 detection
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits at 19:26:02.51 -27:13:10.6: 12.29 +/- 0.03 detection
Forced photometry filter REJECTED candidate at 18:46:48.59 -28:57:34.2: ref_mag=12.86 +/- 0.06 new_mean_mag=12.9291 delta=-0.07 (need > 0.90)
Forced photometry reference-image weighted average: 12.80 +/- 0.04
Forced photometry reference-image weighted average: 12.76 +/- 0.04
Forced photometry reference-image weighted average: 12.93 +/- 0.06
Forced photometry reference-image weighted average: 12.33 +/- 0.03
Forced photometry filter REJECTED candidate at 19:30:23.03 -25:09:59.1: ref_mag=12.80 +/- 0.04 new_mean_mag=13.0855 delta=-0.29 (need > 0.90)
Forced photometry filter REJECTED candidate at 18:51:19.81 -25:36:57.9: ref_mag=12.76 +/- 0.04 new_mean_mag=12.9056 delta=-0.14 (need > 0.90)
Forced photometry filter REJECTED candidate at 18:42:14.56 -27:42:14.2: ref_mag=12.93 +/- 0.06 new_mean_mag=12.8839 delta=0.05 (need > 0.90)
Forced photometry filter REJECTED candidate at 19:26:02.51 -27:13:10.6: ref_mag=12.33 +/- 0.03 new_mean_mag=12.9116 delta=-0.59 (need > 0.90)
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits at 18:49:35.89 -29:06:11.0: 12.83 +/- 0.09 detection
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits at 19:04:40.74 -26:32:27.8: 12.55 +/- 0.04 detection
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits at 18:42:14.92 -27:24:55.6: 12.38 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.03
Forced photometry filter REJECTED candidate at 19:04:40.74 -26:32:27.8: ref_mag=12.56 +/- 0.03 new_mean_mag=12.7727 delta=-0.21 (need > 0.90)
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits at 18:49:35.89 -29:06:11.0: 12.77 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.05
Forced photometry filter REJECTED candidate at 18:49:35.89 -29:06:11.0: ref_mag=12.78 +/- 0.05 new_mean_mag=12.8734 delta=-0.09 (need > 0.90)
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits at 18:49:10.61 -30:00:48.9: 12.82 +/- 0.10 detection
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits at 18:42:14.92 -27:24:55.6: 12.47 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.44 +/- 0.04
Forced photometry filter REJECTED candidate at 18:42:14.92 -27:24:55.6: ref_mag=12.44 +/- 0.04 new_mean_mag=12.6181 delta=-0.18 (need > 0.90)
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits at 19:12:42.89 -29:44:06.6: 12.53 +/- 0.06 detection
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits at 19:02:34.89 -23:03:06.7: 11.23 +/- 0.02 detection
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits at 19:15:43.61 -24:32:29.6: 11.84 +/- 0.03 detection
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits at 18:49:10.61 -30:00:48.9: 12.77 +/- 0.06 detection
Forced photometry reference-image weighted average: 12.78 +/- 0.05
Forced photometry filter REJECTED candidate at 18:49:10.61 -30:00:48.9: ref_mag=12.78 +/- 0.05 new_mean_mag=12.6197 delta=0.16 (need > 0.90)
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits at 19:07:41.21 -28:19:51.0: 10.55 +/- 0.01 detection
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits at 19:12:42.89 -29:44:06.6: 12.53 +/- 0.04 detection
Forced photometry reference-image weighted average: 12.53 +/- 0.03
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits at 18:47:50.41 -28:31:01.0: 14.30 +/- 99.00 upperlimit
Forced photometry filter REJECTED candidate at 19:12:42.89 -29:44:06.6: ref_mag=12.53 +/- 0.03 new_mean_mag=12.7218 delta=-0.19 (need > 0.90)
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits at 19:15:43.61 -24:32:29.6: 11.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 11.81 +/- 0.02
Forced photometry filter REJECTED candidate at 19:15:43.61 -24:32:29.6: ref_mag=11.81 +/- 0.02 new_mean_mag=12.2184 delta=-0.41 (need > 0.90)
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits at 19:02:34.89 -23:03:06.7: 11.41 +/- 0.01 detection
Forced photometry reference-image weighted average: 11.34 +/- 0.01
Forced photometry filter REJECTED candidate at 19:02:34.89 -23:03:06.7: ref_mag=11.34 +/- 0.01 new_mean_mag=11.7798 delta=-0.44 (need > 0.90)
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits at 18:42:57.18 -30:01:01.7: 12.58 +/- 0.09 detection
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits at 19:07:41.21 -28:19:51.0: 10.51 +/- 0.01 detection
Forced photometry reference-image weighted average: 10.52 +/- 0.01
Forced photometry filter REJECTED candidate at 19:07:41.21 -28:19:51.0: ref_mag=10.52 +/- 0.01 new_mean_mag=10.2239 delta=0.30 (need > 0.90)
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits at 18:43:42.85 -28:14:03.2: 12.99 +/- 0.13 detection
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits at 18:47:50.41 -28:31:01.0: 14.73 +/- 99.00 upperlimit
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits at 19:23:01.29 -29:04:20.3: 12.67 +/- 0.08 detection
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits at 18:42:57.18 -30:01:01.7: 12.71 +/- 0.07 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.06
Forced photometry filter REJECTED candidate at 18:42:57.18 -30:01:01.7: ref_mag=12.66 +/- 0.06 new_mean_mag=12.5556 delta=0.10 (need > 0.90)
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits at 19:23:02.36 -22:38:44.3: 14.54 +/- 99.00 upperlimit
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits at 18:44:08.62 -29:11:58.3: 14.17 +/- 99.00 upperlimit
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits at 19:25:31.76 -28:04:12.2: 13.08 +/- 0.10 detection
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits at 18:43:42.85 -28:14:03.2: 13.10 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.06 +/- 0.08
Forced photometry filter REJECTED candidate at 18:43:42.85 -28:14:03.2: ref_mag=13.06 +/- 0.08 new_mean_mag=12.5618 delta=0.50 (need > 0.90)
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits at 18:48:39.35 -27:20:08.1: 12.99 +/- 0.10 detection
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits at 19:23:01.29 -29:04:20.3: 12.66 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.66 +/- 0.04
Forced photometry filter REJECTED candidate at 19:23:01.29 -29:04:20.3: ref_mag=12.66 +/- 0.04 new_mean_mag=12.8351 delta=-0.17 (need > 0.90)
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits at 19:23:02.36 -22:38:44.3: 15.03 +/- 99.00 upperlimit
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits at 18:44:08.62 -29:11:58.3: 14.35 +/- 0.27 detection
Forced photometry reference-image weighted average: 14.35 +/- 0.27
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits at 18:48:48.98 -28:35:44.8: 13.45 +/- 0.16 detection
Forced photometry filter KEPT candidate at 18:44:08.62 -29:11:58.3: ref_mag=14.35 +/- 0.27 new_mean_mag=12.7819 delta=1.57 (need > 0.90)
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits at 19:25:31.76 -28:04:12.2: 12.84 +/- 0.05 detection
Forced photometry reference-image weighted average: 12.89 +/- 0.04
Forced photometry filter REJECTED candidate at 19:25:31.76 -28:04:12.2: ref_mag=12.89 +/- 0.04 new_mean_mag=13.0120 delta=-0.12 (need > 0.90)
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits at 19:02:06.26 -26:53:39.0: 14.52 +/- 99.00 upperlimit
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits at 18:48:39.35 -27:20:08.1: 13.20 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.06
Forced photometry filter REJECTED candidate at 18:48:39.35 -27:20:08.1: ref_mag=13.12 +/- 0.06 new_mean_mag=12.9376 delta=0.18 (need > 0.90)
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits at 18:44:17.36 -26:48:49.9: 13.53 +/- 0.19 detection
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits at 18:48:48.98 -28:35:44.8: 13.31 +/- 0.10 detection
Forced photometry reference-image weighted average: 13.35 +/- 0.08
Forced photometry filter REJECTED candidate at 18:48:48.98 -28:35:44.8: ref_mag=13.35 +/- 0.08 new_mean_mag=13.0727 delta=0.27 (need > 0.90)
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits at 18:45:14.35 -29:55:40.5: 13.51 +/- 0.20 detection
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits at 19:02:06.26 -26:53:39.0: 14.97 +/- 99.00 upperlimit
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits at 18:44:17.36 -26:48:49.9: 13.33 +/- 0.10 detection
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits at 18:41:03.12 -28:09:35.0: 14.14 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.37 +/- 0.09
Forced photometry filter REJECTED candidate at 18:44:17.36 -26:48:49.9: ref_mag=13.37 +/- 0.09 new_mean_mag=13.1613 delta=0.21 (need > 0.90)
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits at 18:44:25.53 -24:20:41.8: 12.94 +/- 0.11 detection
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits at 18:45:14.35 -29:55:40.5: 13.50 +/- 0.13 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.11
Forced photometry filter REJECTED candidate at 18:45:14.35 -29:55:40.5: ref_mag=13.50 +/- 0.11 new_mean_mag=13.1729 delta=0.33 (need > 0.90)
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits at 18:50:19.78 -30:09:14.9: 14.02 +/- 0.29 detection
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits at 18:41:03.12 -28:09:35.0: 14.57 +/- 99.00 upperlimit
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits at 18:44:25.53 -24:20:41.8: 13.24 +/- 0.09 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.07
Forced photometry filter REJECTED candidate at 18:44:25.53 -24:20:41.8: ref_mag=13.12 +/- 0.07 new_mean_mag=13.0934 delta=0.03 (need > 0.90)
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits at 18:50:19.78 -30:09:14.9: 13.94 +/- 0.17 detection
Forced photometry reference-image weighted average: 13.96 +/- 0.15
Forced photometry filter REJECTED candidate at 18:50:19.78 -30:09:14.9: ref_mag=13.96 +/- 0.15 new_mean_mag=13.3854 delta=0.58 (need > 0.90)
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits at 18:42:08.75 -29:37:10.2: 13.40 +/- 0.20 detection
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits at 18:53:01.86 -29:57:05.5: 13.69 +/- 0.21 detection
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits at 18:45:34.63 -29:14:15.5: 13.84 +/- 0.27 detection
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits at 18:42:08.75 -29:37:10.2: 13.49 +/- 0.15 detection
Forced photometry reference-image weighted average: 13.46 +/- 0.12
Forced photometry filter REJECTED candidate at 18:42:08.75 -29:37:10.2: ref_mag=13.46 +/- 0.12 new_mean_mag=13.2160 delta=0.24 (need > 0.90)
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits at 18:41:00.25 -29:12:22.5: 13.29 +/- 0.16 detection
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits at 18:52:15.21 -28:48:22.3: 13.57 +/- 0.19 detection
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits at 18:53:01.86 -29:57:05.5: 13.47 +/- 0.11 detection
Forced photometry reference-image weighted average: 13.52 +/- 0.10
Forced photometry filter REJECTED candidate at 18:53:01.86 -29:57:05.5: ref_mag=13.52 +/- 0.10 new_mean_mag=13.3913 delta=0.12 (need > 0.90)
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits at 18:59:12.64 -24:46:22.9: 14.44 +/- 99.00 upperlimit
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits at 18:41:00.25 -29:12:22.5: 13.62 +/- 0.15 detection
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits at 18:45:34.63 -29:14:15.5: 13.74 +/- 0.15 detection
Forced photometry reference-image weighted average: 13.47 +/- 0.11
Forced photometry reference-image weighted average: 13.77 +/- 0.13
Forced photometry filter REJECTED candidate at 18:45:34.63 -29:14:15.5: ref_mag=13.77 +/- 0.13 new_mean_mag=13.2993 delta=0.47 (need > 0.90)
Forced photometry filter REJECTED candidate at 18:41:00.25 -29:12:22.5: ref_mag=13.47 +/- 0.11 new_mean_mag=13.3407 delta=0.13 (need > 0.90)
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-04-17_04-45-50_20.00sec_-5.00C_LIGHTs_0284.fits at 18:42:53.74 -26:51:37.2: 13.50 +/- 0.18 detection
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits at 18:52:15.21 -28:48:22.3: 13.67 +/- 0.13 detection
Forced photometry reference-image weighted average: 13.64 +/- 0.11
Forced photometry filter REJECTED candidate at 18:52:15.21 -28:48:22.3: ref_mag=13.64 +/- 0.11 new_mean_mag=13.4949 delta=0.14 (need > 0.90)
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits at 18:59:12.64 -24:46:22.9: 14.52 +/- 0.25 detection
Forced photometry reference-image weighted average: 14.52 +/- 0.25
Forced photometry filter KEPT candidate at 18:59:12.64 -24:46:22.9: ref_mag=14.52 +/- 0.25 new_mean_mag=13.4356 delta=1.08 (need > 0.90)
Forced photometry on wcs_Sgr-05-Q2b1x1_2026-07-08_01-16-29_20.00sec_5.00C_LIGHT_0055.fits at 18:42:53.74 -26:51:37.2: 13.87 +/- 0.16 detection
Forced photometry reference-image weighted average: 13.70 +/- 0.12
Forced photometry filter REJECTED candidate at 18:42:53.74 -26:51:37.2: ref_mag=13.70 +/- 0.12 new_mean_mag=13.3753 delta=0.33 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out129336.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129374.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129388.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129482.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out129303.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out129334.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 9s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 129118_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129118_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
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Considering the candidate 129132_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129132_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
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Considering the candidate 129133_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129133_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (21.4") between the two second-epoch detections
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Considering the candidate 129150_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129150_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
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Considering the candidate 129152_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129152_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
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Considering the candidate 129156_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129156_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
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Considering the candidate 129158_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129158_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
**** FOUND 18:59:04.10 -24:17:35.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 129160_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129160_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
**** FOUND 19:20:36.85 -22:10:03.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 129161_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129161_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
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Considering the candidate 129164_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129164_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
**** FOUND 18:59:42.81 -30:14:39.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 129170_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129170_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
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Considering the candidate 129185_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129185_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
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Considering the candidate 129190_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129190_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
**** FOUND 19:20:58.06 -26:11:46.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 129191_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129191_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
**** FOUND 19:22:56.23 -25:13:11.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 129203_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129203_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
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Considering the candidate 129206_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129206_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
**** FOUND 19:10:39.88 -26:18:36.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 129211_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129211_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
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Considering the candidate 129212_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129212_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
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Considering the candidate 129213_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129213_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
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Considering the candidate 129218_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129218_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
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Considering the candidate 129219_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129219_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
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Considering the candidate 129221_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129221_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
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Considering the candidate 129227_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129227_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
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Considering the candidate 129232_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129232_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
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Considering the candidate 129233_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129233_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (15.4") between the two second-epoch detections
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Considering the candidate 129236_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129236_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
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Considering the candidate 129244_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129244_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
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Considering the candidate 129245_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129245_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
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Considering the candidate 129258_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129258_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
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Considering the candidate 129270_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129270_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
**** FOUND 18:52:48.75 -27:19:10.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 129278_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129278_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
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Considering the candidate 129280_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129280_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
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Considering the candidate 129285_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129285_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
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Considering the candidate 129290_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129290_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
**** FOUND 19:00:33.52 -22:13:03.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 129291_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129291_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
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Considering the candidate 129294_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129294_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
**** FOUND 18:50:01.09 -23:33:28.5 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 129303_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
Preparing report for the candidate 129303_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
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Considering the candidate 129312_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129312_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
**** FOUND 19:21:22.68 -29:30:50.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 129313_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129313_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
**** FOUND 18:44:57.59 -27:38:30.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 129321_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129321_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
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Considering the candidate 129322_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129322_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
**** FOUND 18:51:43.38 -29:00:35.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 129328_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129328_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
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Considering the candidate 129330_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129330_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
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Considering the candidate 129332_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129332_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
**** FOUND 18:44:01.18 -30:01:42.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 129334_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
Preparing report for the candidate 129334_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
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Considering the candidate 129336_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129336_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
**** FOUND 18:44:08.62 -29:11:58.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.78, MAG_FAINT_SEARCH_LIMIT=13.76)GAIADR2_OUTPUT=# 1.370 4071341439958402304 281.03548297504 -29.19948884089 12.5278 10.6717 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.370#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129337_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129337_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
**** FOUND 19:09:09.22 -23:24:40.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 129341_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129341_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
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Considering the candidate 129343_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129343_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
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Considering the candidate 129350_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129350_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
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Considering the candidate 129374_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129374_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
**** FOUND 19:02:06.26 -26:53:39.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 4.435 6763718178541730688 285.52694848938 -26.89320629063 12.3204 10.2183 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.435#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129377_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129377_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
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Considering the candidate 129378_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129378_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
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Considering the candidate 129388_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129388_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
**** FOUND 18:41:03.12 -28:09:35.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 0.950 4072417724402243712 280.26289476215 -28.15996936941 13.3598 11.4896 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.950#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129395_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129395_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
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Considering the candidate 129405_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129405_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
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Considering the candidate 129411_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129411_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
Rejecting candidate due to large distance (22.9") between the two second-epoch detections
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Considering the candidate 129413_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129413_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
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Considering the candidate 129417_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129417_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
**** FOUND 19:25:29.80 -24:20:13.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 129418_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129418_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
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Considering the candidate 129434_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129434_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
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Considering the candidate 129438_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129438_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
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Considering the candidate 129463_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129463_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
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Considering the candidate 129482_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129482_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
**** FOUND 18:59:12.64 -24:46:22.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 1.866 4074380460047972352 284.80319020473 -24.77323455208 14.0109 13.4946 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.866#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129524_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 129524_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
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Considering the candidate 96283_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 96283_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
**** FOUND 18:54:20.97 -26:02:20.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 97481_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 97481_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
**** FOUND 18:47:33.74 -24:07:20.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 97601_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 97601_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
**** FOUND 19:18:59.45 -23:54:30.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 101263_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 101263_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
**** FOUND 19:13:49.90 -22:29:07.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 97101_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 97101_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks
**** FOUND 19:10:50.53 -23:55:19.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 96831_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015
The candidate 96831_fd_Sgr-05-Q2b1x1_2026-08-02_21-50-01_20.00sec_-0.00C_LIGHT_0015 did not pass the final checks