This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 28.3876* 04 10 19.30 +20 53 16.4 7.5 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461249.8876,7.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260728.3876 7.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 07 28.3876* 04 10 19.29 +20 53 16.5 7.7 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461249.8876,7.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260728.3876 7.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 28.3876 2461249.8876 12.51 04:21:23.23 +26:17:23.3
170.80807 -16.49491 galactic Tau Second-epoch detections are separated by 0.3" and 8.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.63 Ausonia -0 -0 0 12.6 0 0
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:21:23.23 +26:17:23.3: 16.21 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits at 04:21:23.23 +26:17:23.3: 16.23 +/- 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!
TCP 2026 07 28.3876* 04 21 23.23 +26 17 23.3 12.5 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461249.8876,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260728.3876 12.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 28.3876 2461249.8876 13.15 04:39:30.60 +21:51:22.3
177.12216 -16.25485 galactic Tau Second-epoch detections are separated by 2.8" and 8.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.110 Lydia 0 0 0 13.4 0 0
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:39:30.60 +21:51:22.3: 16.39 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits at 04:39:30.60 +21:51:22.3: 16.35 +/- 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!
TCP 2026 07 28.3876* 04 39 30.60 +21 51 22.3 13.2 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461249.8876,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260728.3876 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.68987713 09.01.2026 04:33:15.384 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
First image: 2461049.68987713 09.01.2026 04:33:15.384 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Last image: 2461249.88799721 28.07.2026 09:18:32.959 /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.50
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
Total objects detected (at least 2 times): 11261
Objects passed selection criteria: 11183
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 7295
Average stars matched: 7090 (97.1899 %)
Memory usage VmPeak: 237152 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Jul 28 02:13:30 CDT 2026
VaST build number 1.0rc89-182-g8380f0ac
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-28)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Jul 28 07:26:07 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: 2461049.68987713 09.01.2026 04:33:15.384 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
First image: 2461049.68987713 09.01.2026 04:33:15.384 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Last image: 2461249.88799721 28.07.2026 09:18:32.959 /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 29
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.21
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: 18 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
Total objects detected (at least 2 times): 78484
Objects passed selection criteria: 78267
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 52667.2
Average stars matched: 50793.5 (96.4423 %)
Memory usage VmPeak: 298360 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Jul 28 02:13:30 CDT 2026
VaST build number 1.0rc89-182-g8380f0ac
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-28)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Jul 28 07:30:17 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/TTUQ1b1x1/TTUQ1_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/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits
SExtractor catalog cache: saved Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.cat to cache
SExtractor catalog cache: saved Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.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/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.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: 2461249.88727590
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_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits exists and is non-empty
Saving wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits to local_wcs_cache/
'wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits' -> 'local_wcs_cache/wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits'
wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits exists and is non-empty
Saving wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits to local_wcs_cache/
'wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits' -> 'local_wcs_cache/wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits'
wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits exists and is non-empty
Saving wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits to local_wcs_cache/
'wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits' -> 'local_wcs_cache/wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits'
wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits exists and is non-empty
Saving wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits to local_wcs_cache/
'wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits' -> 'local_wcs_cache/wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits (1st reference image)
verification OK: wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Image size: 941.4'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 04:36:56.001 +21:59:37.88 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_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits (1st new image)
verification OK: wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits
Image size: 945.0'x626.9' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 04:36:54.787 +22:00:52.36 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 04:36:56.001 +21:59:37.88
Second-epoch image center 04:36:54.787 +22:00:52.36
Angular distance between the image centers 0.0212 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits (2nd new image)
verification OK: wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits
Image size: 944.9'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 04:36:52.101 +22:00:19.18 J2000 4789.000 3195.000
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# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 04:36:56.001 +21:59:37.88
Second-epoch image center 04:36:52.101 +22:00:19.18
Angular distance between the image centers 0.0189 deg.
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# 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 04:36:54.787 +22:00:52.36
Second-epoch second image center 04:36:52.101 +22:00:19.18
Angular distance between the image centers 0.01388 deg.
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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/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits &> /tmp/tmp.50kTPfateV
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits &> /tmp/tmp.BsoRVmp48r
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits &> /tmp/tmp.L2z3ACBLgv
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits &> /tmp/tmp.9LWgg22AT6
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.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_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits and wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.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_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits and wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat
Found non-empty wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits and wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat
The reference image (wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits) and catalog (wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat) found
'wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat' -> 'wcsmag.cat'
Read 11927 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 60.5122 to 78.0896 deg, Dec +16.4863 to +27.2832 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 60.5122 to 78.0896 deg, Dec 16.4863 to 27.2832 deg
Loaded 5179 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): 3947 out of 4318 total matches.
Matched with Tycho-2 4318 out of 11927 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.997000
a=0.000000 b=1.000000 c=22.997000
From vast_summary.log: estimated ref. image limiting mag.: -7.50
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.50
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.50
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 11927 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 60.5122 to 78.0896 deg, Dec +16.4863 to +27.2832 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 60.5122 to 78.0896 deg, Dec 16.4863 to 27.2832 deg
Loaded 5179 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): 3947 out of 4318 total matches.
Matched with Tycho-2 4318 out of 11927 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits:
Forced-photometry filter: calibrated wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits -> calib.txt_param_ref_wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits (aperture=6.0)
Read 12023 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 60.5322 to 78.0896 deg, Dec +16.4883 to +27.2799 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 60.5322 to 78.0896 deg, Dec 16.4883 to 27.2799 deg
Loaded 5164 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): 3942 out of 4310 total matches.
Matched with Tycho-2 4310 out of 12023 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits:
Forced-photometry filter: calibrated wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits -> calib.txt_param_ref_wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits (aperture=6.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
2.0 pix Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
2.5 pix fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits
2.5 pix fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits
2.0 pix wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
2.0 pix wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
Limiting magnitude estimates:
15.5 mag. Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
15.5 mag. Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
13.4 mag. fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits
13.3 mag. fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits
All-image limiting magnitude estimate: 13.3 (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.50kTPfateV (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_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits' -> 'wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.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/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
WCS_IMAGE_NAME=wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
WCS-calibrated image found: wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Checking if the catalog wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat corresponding to the image wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits alredy exist and is non-empty...
Catalog wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat corresponding to the image wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
WCS catalog name: wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=967, bad_region=0, passed=11927
Got 11927 stars (including 10942 good ones) from the SExtractor catalog wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat
util/solve_plate_with_UCAC5 got 11927 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4867 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4845 matched stars entering correct_measured_positions(), 4845 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4845 matched stars entering correct_measured_positions(), 11927 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4866 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4844 matched stars entering correct_measured_positions(), 11927 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4844 matched stars entering correct_measured_positions(), 11927 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4844 stars left (next iteration limit 5329)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits N_match=4844 sigma_overall_arcsec=0.304 sigma_q1_arcsec=0.379 sigma_q2_arcsec=0.308 sigma_q3_arcsec=0.266 sigma_q4_arcsec=0.252 n_q1=1283 n_q2=1077 n_q3=1448 n_q4=1036 worst_quadrant_to_overall_ratio=1.249
The image catalog is written to wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits -region wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.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.BsoRVmp48r (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_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits' -> 'wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.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/Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
WCS_IMAGE_NAME=wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
WCS-calibrated image found: wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
Checking if the catalog wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits.wcscat corresponding to the image wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits alredy exist and is non-empty...
Catalog wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits.wcscat corresponding to the image wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
WCS catalog name: wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=981, bad_region=0, passed=12023
Got 12023 stars (including 11026 good ones) from the SExtractor catalog wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits.wcscat
util/solve_plate_with_UCAC5 got 12023 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4870 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4848 matched stars entering correct_measured_positions(), 4848 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4848 matched stars entering correct_measured_positions(), 12023 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4868 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4847 matched stars entering correct_measured_positions(), 12023 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4847 matched stars entering correct_measured_positions(), 12023 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 4847 stars left (next iteration limit 5332)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits N_match=4847 sigma_overall_arcsec=0.302 sigma_q1_arcsec=0.404 sigma_q2_arcsec=0.314 sigma_q3_arcsec=0.249 sigma_q4_arcsec=0.248 n_q1=1282 n_q2=1079 n_q3=1442 n_q4=1044 worst_quadrant_to_overall_ratio=1.336
The image catalog is written to wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits -region wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.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.L2z3ACBLgv (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_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits
WCS_IMAGE_NAME=wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits
WCS-calibrated image found: wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits
Checking if the catalog wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits.wcscat corresponding to the image wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits.wcscat corresponding to the image wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits
WCS catalog name: wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=234, bad_region=0, passed=2712
Got 2712 stars (including 2474 good ones) from the SExtractor catalog wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits.wcscat
util/solve_plate_with_UCAC5 got 2712 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 945.0'
Seting catalog search parameters based on the expected field of view 945.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013125 (47.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010500 (37.8 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 530 to 589 (Dec 16.2 to 27.5)
Done reading UCAC5 zone files...
Matched 2407 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2399 matched stars entering correct_measured_positions(), 2399 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2399 matched stars entering correct_measured_positions(), 2712 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 530 to 589 (Dec 16.2 to 27.5)
Done reading UCAC5 zone files...
Matched 2405 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2398 matched stars entering correct_measured_positions(), 2712 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 2398 matched stars entering correct_measured_positions(), 2712 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 2398 stars left (next iteration limit 2638)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=2398 robust_rms=9.190 arcsec worst_quadrant_rms=10.896 arcsec
SIP_REFIT: SIP order 3 trial: matched=2398 robust_rms=0.659 arcsec worst_quadrant_rms=0.989 arcsec
SIP_REFIT: SIP order 5 trial: matched=2398 robust_rms=0.392 arcsec worst_quadrant_rms=0.484 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=2398 robust_rms_before=1.576 arcsec robust_rms_before_corrected=0.389 arcsec robust_rms_after=0.392 arcsec worst_quadrant_rms_before=0.495 worst_quadrant_rms_after=0.484
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.495 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits N_match=2398 sigma_overall_arcsec=0.400 sigma_q1_arcsec=0.390 sigma_q2_arcsec=0.461 sigma_q3_arcsec=0.348 sigma_q4_arcsec=0.404 n_q1=609 n_q2=602 n_q3=562 n_q4=625 worst_quadrant_to_overall_ratio=1.151
The image catalog is written to wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits -region wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.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.9LWgg22AT6 (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_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.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_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits
WCS_IMAGE_NAME=wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits
WCS-calibrated image found: wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits
Checking if the catalog wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits.wcscat corresponding to the image wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits.wcscat corresponding to the image wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits
WCS catalog name: wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=241, bad_region=0, passed=2703
Got 2703 stars (including 2457 good ones) from the SExtractor catalog wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits.wcscat
util/solve_plate_with_UCAC5 got 2703 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.9'
Seting catalog search parameters based on the expected field of view 944.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013124 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010499 (37.8 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 530 to 589 (Dec 16.2 to 27.5)
Done reading UCAC5 zone files...
Matched 2392 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2384 matched stars entering correct_measured_positions(), 2384 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 2384 matched stars entering correct_measured_positions(), 2703 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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 530 to 589 (Dec 16.2 to 27.5)
Done reading UCAC5 zone files...
Matched 2392 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 2385 matched stars entering correct_measured_positions(), 2703 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 2385 matched stars entering correct_measured_positions(), 2703 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 2385 stars left (next iteration limit 2622)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=2385 robust_rms=10.078 arcsec worst_quadrant_rms=11.122 arcsec
SIP_REFIT: SIP order 3 trial: matched=2385 robust_rms=0.583 arcsec worst_quadrant_rms=0.934 arcsec
SIP_REFIT: SIP order 5 trial: matched=2385 robust_rms=0.385 arcsec worst_quadrant_rms=0.513 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=2385 robust_rms_before=1.541 arcsec robust_rms_before_corrected=0.390 arcsec robust_rms_after=0.385 arcsec worst_quadrant_rms_before=0.471 worst_quadrant_rms_after=0.513
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.471 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits N_match=2385 sigma_overall_arcsec=0.397 sigma_q1_arcsec=0.355 sigma_q2_arcsec=0.467 sigma_q3_arcsec=0.368 sigma_q4_arcsec=0.400 n_q1=611 n_q2=617 n_q3=540 n_q4=617 worst_quadrant_to_overall_ratio=1.176
The image catalog is written to wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits -region wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.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=Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits sigma_overall=0.304 worst_q_ratio=1.249
ref2=Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits sigma_overall=0.302 worst_q_ratio=1.336
new1=fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits sigma_overall=0.400 worst_q_ratio=1.151
new2=fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits sigma_overall=0.397 worst_q_ratio=1.176
reference average sigma_overall=0.303 worst_q_ratio=1.2925
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161_astrometric_residuals.png (4844 matched stars from wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162_astrometric_residuals.png (4847 matched stars from wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412_astrometric_residuals.png (2398 matched stars from wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.36 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413_astrometric_residuals.png (2385 matched stars from wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.36 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits'
Saving fully-calibrated image wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits'
Preparing the HTML report for the field Tau-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 2s
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 20746_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413
The candidate 20746_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413 did not pass the final checks
**** FOUND 04:23:57.79 +24:18:12.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20748_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413
Preparing report for the candidate 20748_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 3s
Prepared the HTML report for the field Tau-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
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/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits
SExtractor catalog cache: saved Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.cat to cache
SExtractor catalog cache: saved Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Creating symlink local_wcs_cache/wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.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_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits exists and is non-empty
wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits exists and is non-empty
wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits exists and is non-empty
wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits (1st reference image)
verification OK: wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Image size: 941.4'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 04:36:56.001 +21:59:37.88 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_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits (1st new image)
verification OK: wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits
Image size: 945.0'x626.9' 15.8(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 04:36:54.787 +22:00:52.36 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 04:36:56.001 +21:59:37.88
Second-epoch image center 04:36:54.787 +22:00:52.36
Angular distance between the image centers 0.0212 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits (2nd new image)
verification OK: wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits
Image size: 944.9'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 04:36:52.101 +22:00:19.18 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 04:36:56.001 +21:59:37.88
Second-epoch image center 04:36:52.101 +22:00:19.18
Angular distance between the image centers 0.0189 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 04:36:54.787 +22:00:52.36
Second-epoch second image center 04:36:52.101 +22:00:19.18
Angular distance between the image centers 0.01388 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/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits &> /tmp/tmp.dY7Xz7RZ7G
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits &> /tmp/tmp.1gkEs3XmEf
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits &> /tmp/tmp.WT0lVVJCqV
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits &> /tmp/tmp.qFenw4jOEx
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.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_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits and wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.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_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits and wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat
Found non-empty wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits and wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat
The reference image (wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits) and catalog (wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat) found
'wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat' -> 'wcsmag.cat'
Read 86341 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 60.5077 to 78.1095 deg, Dec +16.4682 to +27.2856 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 60.5077 to 78.1095 deg, Dec 16.4682 to 27.2856 deg
Loaded 5191 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): 3474 out of 4349 total matches.
Matched with Tycho-2 4349 out of 86341 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.857050
a=0.000000 b=1.000000 c=22.857050
From vast_summary.log: estimated ref. image limiting mag.: -7.21
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.65
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.65
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 86341 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 60.5077 to 78.1095 deg, Dec +16.4682 to +27.2856 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 60.5077 to 78.1095 deg, Dec 16.4682 to 27.2856 deg
Loaded 5191 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): 3474 out of 4349 total matches.
Matched with Tycho-2 4349 out of 86341 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits:
Forced-photometry filter: calibrated wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits -> calib.txt_param_ref_wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits (aperture=4.5)
Read 85691 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 60.5078 to 78.1091 deg, Dec +16.4883 to +27.2975 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 60.5078 to 78.1091 deg, Dec 16.4883 to 27.2975 deg
Loaded 5188 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): 3464 out of 4347 total matches.
Matched with Tycho-2 4347 out of 85691 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits:
Forced-photometry filter: calibrated wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits -> calib.txt_param_ref_wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits (aperture=4.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 29 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
1.9 pix Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
2.4 pix fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits
2.4 pix fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits
1.9 pix wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
1.9 pix wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
Limiting magnitude estimates:
15.7 mag. Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
15.6 mag. Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
13.5 mag. fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits
13.5 mag. fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits
All-image limiting magnitude estimate: 13.5 (SNR ) 13.1 (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.dY7Xz7RZ7G (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_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits' -> 'wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.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/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
WCS_IMAGE_NAME=wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
WCS-calibrated image found: wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
Checking if the catalog wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat corresponding to the image wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits alredy exist and is non-empty...
Catalog wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat corresponding to the image wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits
WCS catalog name: wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=23, blended=6242, bad_region=8, passed=86318
Got 86318 stars (including 79890 good ones) from the SExtractor catalog wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat
util/solve_plate_with_UCAC5 got 86318 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4869 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4857 matched stars entering correct_measured_positions(), 4857 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4857 matched stars entering correct_measured_positions(), 86318 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4868 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4857 matched stars entering correct_measured_positions(), 86318 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4857 matched stars entering correct_measured_positions(), 86318 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 4857 stars left (next iteration limit 5342)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits N_match=4857 sigma_overall_arcsec=0.301 sigma_q1_arcsec=0.390 sigma_q2_arcsec=0.290 sigma_q3_arcsec=0.279 sigma_q4_arcsec=0.255 n_q1=1260 n_q2=1091 n_q3=1439 n_q4=1067 worst_quadrant_to_overall_ratio=1.297
The image catalog is written to wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits -region wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.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.1gkEs3XmEf (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_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits' -> 'wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.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/Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
WCS_IMAGE_NAME=wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
WCS-calibrated image found: wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
Checking if the catalog wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits.wcscat corresponding to the image wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits alredy exist and is non-empty...
Catalog wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits.wcscat corresponding to the image wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits
WCS catalog name: wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=19, blended=6215, bad_region=8, passed=85672
Got 85672 stars (including 79297 good ones) from the SExtractor catalog wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits.wcscat
util/solve_plate_with_UCAC5 got 85672 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4873 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4860 matched stars entering correct_measured_positions(), 4860 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4860 matched stars entering correct_measured_positions(), 85672 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
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 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 4873 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4860 matched stars entering correct_measured_positions(), 85672 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4860 matched stars entering correct_measured_positions(), 85672 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4860 stars left (next iteration limit 5346)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits N_match=4860 sigma_overall_arcsec=0.289 sigma_q1_arcsec=0.389 sigma_q2_arcsec=0.290 sigma_q3_arcsec=0.258 sigma_q4_arcsec=0.236 n_q1=1254 n_q2=1089 n_q3=1441 n_q4=1076 worst_quadrant_to_overall_ratio=1.345
The image catalog is written to wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits -region wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.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.WT0lVVJCqV (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_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits
WCS_IMAGE_NAME=wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits
WCS-calibrated image found: wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits
Checking if the catalog wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits.wcscat corresponding to the image wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits.wcscat corresponding to the image wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits
WCS catalog name: wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=2, blended=543, bad_region=2, passed=19948
Got 19948 stars (including 19374 good ones) from the SExtractor catalog wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits.wcscat
util/solve_plate_with_UCAC5 got 19948 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 945.0'
Seting catalog search parameters based on the expected field of view 945.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013125 (47.3 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010500 (37.8 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 530 to 589 (Dec 16.1 to 27.5)
Done reading UCAC5 zone files...
Matched 4863 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4841 matched stars entering correct_measured_positions(), 4841 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4841 matched stars entering correct_measured_positions(), 19948 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 530 to 589 (Dec 16.1 to 27.5)
Done reading UCAC5 zone files...
Matched 4860 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4842 matched stars entering correct_measured_positions(), 19948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 4842 matched stars entering correct_measured_positions(), 19948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 4842 stars left (next iteration limit 5325)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits N_match=4842 sigma_overall_arcsec=0.432 sigma_q1_arcsec=0.415 sigma_q2_arcsec=0.499 sigma_q3_arcsec=0.365 sigma_q4_arcsec=0.446 n_q1=1212 n_q2=1157 n_q3=1166 n_q4=1307 worst_quadrant_to_overall_ratio=1.155
The image catalog is written to wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits -region wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.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.qFenw4jOEx (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_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.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_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits
WCS_IMAGE_NAME=wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits
WCS-calibrated image found: wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits
Checking if the catalog wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits.wcscat corresponding to the image wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits.wcscat corresponding to the image wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits
WCS catalog name: wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 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=4, blended=559, bad_region=1, passed=20118
Got 20118 stars (including 19529 good ones) from the SExtractor catalog wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits.wcscat
util/solve_plate_with_UCAC5 got 20118 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.9'
Seting catalog search parameters based on the expected field of view 944.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013124 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010499 (37.8 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 530 to 589 (Dec 16.1 to 27.5)
Done reading UCAC5 zone files...
Matched 4856 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4834 matched stars entering correct_measured_positions(), 4834 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4834 matched stars entering correct_measured_positions(), 20118 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 530 to 589 (Dec 16.1 to 27.5)
Done reading UCAC5 zone files...
Matched 4854 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(), 20118 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 4834 matched stars entering correct_measured_positions(), 20118 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 4834 stars left (next iteration limit 5317)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits N_match=4834 sigma_overall_arcsec=0.430 sigma_q1_arcsec=0.396 sigma_q2_arcsec=0.522 sigma_q3_arcsec=0.377 sigma_q4_arcsec=0.442 n_q1=1195 n_q2=1181 n_q3=1150 n_q4=1308 worst_quadrant_to_overall_ratio=1.215
The image catalog is written to wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits -region wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.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_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-17-30_20.00sec_-0.00C_LIGHTs_0412.fits
Saving fully-calibrated image wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.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_2026-07-28_CI_Tau-03-Q1b1x1_051421_TTUQ1b1x1_432044_Xiqj4dBI/wcs_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413.fits
Preparing the HTML report for the field Tau-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:21:45.28 +19:28:44.6: 12.50 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:14:36.79 +20:32:28.7: 13.21 +/- 0.02 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:12:41.58 +23:31:30.3: 12.73 +/- 0.02 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:21:23.23 +26:17:23.3: 16.21 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 05:06:29.79 +16:30:55.4: 99.00 +/- 99.00 edge
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits at 04:21:45.28 +19:28:44.6: 12.50 +/- 0.01 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits at 05:06:29.79 +16:30:55.4: 99.00 +/- 99.00 edge
Forced photometry filter REJECTED candidate at 05:06:29.79 +16:30:55.4: at least one reference image reported edge (off-image or aperture/annulus past image boundary); cannot perform the forced-photometry cross-check
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits at 04:21:23.23 +26:17:23.3: 16.23 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.50 +/- 0.01
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits at 04:12:41.58 +23:31:30.3: 12.78 +/- 0.02 detection
Forced photometry filter REJECTED candidate at 04:21:45.28 +19:28:44.6: ref_mag=12.50 +/- 0.01 new_mean_mag=12.2948 delta=0.21 (need > 0.90)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits at 04:14:36.79 +20:32:28.7: 13.17 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.01
Forced photometry filter REJECTED candidate at 04:12:41.58 +23:31:30.3: ref_mag=12.75 +/- 0.01 new_mean_mag=12.6073 delta=0.14 (need > 0.90)
Forced photometry reference-image weighted average: 13.19 +/- 0.02
Forced photometry filter REJECTED candidate at 04:14:36.79 +20:32:28.7: ref_mag=13.19 +/- 0.02 new_mean_mag=12.8312 delta=0.36 (need > 0.90)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:48:48.91 +21:18:40.7: 12.74 +/- 0.02 detection
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-15_20.00sec_-14.90C_LIGHT_0161.fits at 04:39:30.60 +21:51:22.3: 16.39 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits at 04:48:48.91 +21:18:40.7: 12.71 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.73 +/- 0.01
Forced photometry filter REJECTED candidate at 04:48:48.91 +21:18:40.7: ref_mag=12.73 +/- 0.01 new_mean_mag=12.5372 delta=0.19 (need > 0.90)
Forced photometry on wcs_Tau-03-Q1b1x1_2026-01-08_22-33-56_20.00sec_-14.90C_LIGHT_0162.fits at 04:39:30.60 +21:51:22.3: 16.35 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out103528.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103729.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 8s
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: 2s
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Considering the candidate 103334_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413
The candidate 103334_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413 did not pass the final checks
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Considering the candidate 103335_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413
The candidate 103335_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413 did not pass the final checks
**** FOUND 04:26:06.07 +22:54:24.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103336_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413
The candidate 103336_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413 did not pass the final checks
**** FOUND 04:23:57.76 +24:18:13.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 103338_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413
Preparing report for the candidate 103338_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413
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Considering the candidate 103403_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413
The candidate 103403_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413 did not pass the final checks
**** FOUND 04:28:23.70 +19:10:45.7 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 103405_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413
The candidate 103405_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413 did not pass the final checks
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Considering the candidate 103521_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413
The candidate 103521_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413 did not pass the final checks
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Considering the candidate 103528_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413
Preparing report for the candidate 103528_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413
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Considering the candidate 103554_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413
The candidate 103554_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413 did not pass the final checks
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Considering the candidate 103570_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413
The candidate 103570_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413 did not pass the final checks
**** FOUND 04:38:26.86 +26:55:00.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 103590_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413
The candidate 103590_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413 did not pass the final checks
**** FOUND 04:10:47.89 +18:26:18.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103591_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413
The candidate 103591_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413 did not pass the final checks
**** FOUND 04:42:09.68 +22:55:08.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103598_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413
The candidate 103598_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413 did not pass the final checks
**** FOUND 04:26:29.13 +22:48:44.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103605_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413
The candidate 103605_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413 did not pass the final checks
**** FOUND 04:26:10.67 +22:49:27.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 103635_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413
The candidate 103635_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413 did not pass the final checks
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Considering the candidate 103658_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413
The candidate 103658_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413 did not pass the final checks
**** FOUND 04:34:38.49 +22:42:10.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103695_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413
The candidate 103695_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413 did not pass the final checks
**** FOUND 04:27:17.97 +23:01:29.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 103722_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413
The candidate 103722_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413 did not pass the final checks
**** FOUND 04:25:20.68 +22:10:31.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103729_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413
Preparing report for the candidate 103729_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413
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Considering the candidate 103738_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413
The candidate 103738_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413 did not pass the final checks
**** FOUND 04:32:38.87 +23:58:26.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103748_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413
The candidate 103748_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413 did not pass the final checks
**** FOUND 04:28:14.33 +24:06:09.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58469_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413
The candidate 58469_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413 did not pass the final checks
**** FOUND 04:52:47.03 +17:16:29.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53022_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413
The candidate 53022_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413 did not pass the final checks
**** FOUND 04:58:39.91 +20:57:06.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 36988_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413
The candidate 36988_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413 did not pass the final checks
**** FOUND 04:46:31.90 +22:41:09.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 06030_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413
The candidate 06030_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413 did not pass the final checks
**** FOUND 04:46:44.53 +26:23:07.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52280_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413
The candidate 52280_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413 did not pass the final checks
**** FOUND 04:15:01.06 +21:09:09.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 46659_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413
The candidate 46659_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413 did not pass the final checks
**** FOUND 04:34:42.91 +21:46:21.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 35380_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413
The candidate 35380_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413 did not pass the final checks
**** FOUND 04:44:21.49 +22:50:08.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 05458_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413
The candidate 05458_fd_Tau-03-Q1b1x1_2026-07-28_04-18-32_20.00sec_-0.00C_LIGHTs_0413 did not pass the final checks