This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 07 30.3431 2461251.8431 11.84 03:50:40.92 +23:42:09.2
167.55055 -23.25522 galactic Tau Second-epoch detections are separated by 0.5" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.230 Athamantis 0 1 1 12.3 0 0
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:50:40.92 +23:42:09.2: 16.26 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:50:40.92 +23:42:09.2: 16.29 +/- 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 30.3431* 03 50 40.92 +23 42 09.2 11.8 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,2461251.8431,11.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260730.3431 11.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3431 2461251.8431 12.52 03:43:55.82 +22:36:35.6
167.11015 -25.11018 galactic Tau Second-epoch detections are separated by 1.1" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.49 Pales 0 -0 0 13.1 0 0
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:43:55.82 +22:36:35.6: 16.32 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:43:55.82 +22:36:35.6: 16.30 +/- 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 30.3431* 03 43 55.82 +22 36 35.6 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,2461251.8431,12.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260730.3431 12.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 07 30.3431 2461251.8431 12.25 03:43:21.20 +18:01:20.9
170.50181 -28.56113 galactic Tau Second-epoch detections are separated by 1.0" and 6.1 pix
The object was found in VSX 2" HAT 307-0000152
Type: ROT
# Max. Min./Amp. JD0 Period
6.630 J Y 0.193 r 72.624365560000
The object was not found in astcheck.
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:43:21.20 +18:01:20.9: 13.09 +/- 0.02 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:43:21.20 +18:01:20.9: 13.15 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.01
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 30.3431* 03 43 21.20 +18 01 20.9 12.2 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
HAT 307-0000152,2461251.8431,12.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HAT 307-0000152 20260730.3431 12.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.67777097 09.01.2026 04:15:49.412 /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
First image: 2461049.67777097 09.01.2026 04:15:49.412 /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
Last image: 2461251.84337593 30.07.2026 08:14:17.680 /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.51
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: 2 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 8930
Objects passed selection criteria: 8874
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 5300
Average stars matched: 5051.5 (95.3113 %)
Memory usage VmPeak: 235276 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 29 18:03:05 CDT 2026
VaST build number 1.0rc89-187-gf9db235a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-29)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Jul 30 04:48:16 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: 2461049.67777097 09.01.2026 04:15:49.412 /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
First image: 2461049.67777097 09.01.2026 04:15:49.412 /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
Last image: 2461251.84337593 30.07.2026 08:14:17.680 /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 11
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.20
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: 9 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 57312
Objects passed selection criteria: 57109
Measurements per detected object (mean, median, min, max): 2.3 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.3 2.0 2 4
Average stars detected per image: 35984.5
Average stars matched: 33868 (94.1183 %)
Memory usage VmPeak: 279480 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Jul 29 18:03:05 CDT 2026
VaST build number 1.0rc89-187-gf9db235a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-07-29)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Jul 30 04:48:55 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits
SExtractor catalog cache: saved Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.cat to cache
SExtractor catalog cache: saved Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.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-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.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: 2461251.84290356
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-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits exists and is non-empty
Saving wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits to local_wcs_cache/
'wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits' -> 'local_wcs_cache/wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits'
wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits exists and is non-empty
Saving wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits to local_wcs_cache/
'wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits' -> 'local_wcs_cache/wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits'
wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits exists and is non-empty
Saving wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits to local_wcs_cache/
'wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits' -> 'local_wcs_cache/wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits'
wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits exists and is non-empty
Saving wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits to local_wcs_cache/
'wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits' -> 'local_wcs_cache/wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits (1st reference image)
verification OK: wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
Image size: 941.4'x626.9' 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: 03:41:33.240 +21:59:53.22 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-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits (1st new image)
verification OK: wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits
Image size: 940.9'x624.4' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 03:41:31.848 +22:00:04.98 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 03:41:33.240 +21:59:53.22
Second-epoch image center 03:41:31.848 +22:00:04.98
Angular distance between the image centers 0.0063 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits (2nd new image)
verification OK: wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits
Image size: 940.9'x624.4' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 03:41:34.409 +22:00:04.90 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 03:41:33.240 +21:59:53.22
Second-epoch image center 03:41:34.409 +22:00:04.90
Angular distance between the image centers 0.0056 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 03:41:31.848 +22:00:04.98
Second-epoch second image center 03:41:34.409 +22:00:04.90
Angular distance between the image centers 0.00989 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-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits &> /tmp/tmp.ZIi1Of5a3d
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits &> /tmp/tmp.tQFoSpDJ5m
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits &> /tmp/tmp.0SnQTv0TIo
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits &> /tmp/tmp.3wTgKObUK6
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.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-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits and wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.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-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits and wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.wcscat
Found non-empty wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits and wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.wcscat
The reference image (wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits) and catalog (wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.wcscat) found
'wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.wcscat' -> 'wcsmag.cat'
Read 11324 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 46.6722 to 64.2527 deg, Dec +16.5358 to +27.2945 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 46.6722 to 64.2527 deg, Dec 16.5358 to 27.2945 deg
Loaded 6126 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): 4792 out of 5149 total matches.
Matched with Tycho-2 5149 out of 11324 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.940200
a=0.000000 b=1.000000 c=22.940200
From vast_summary.log: estimated ref. image limiting mag.: -7.51
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.43
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.43
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 11324 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 46.6722 to 64.2527 deg, Dec +16.5358 to +27.2945 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 46.6722 to 64.2527 deg, Dec 16.5358 to 27.2945 deg
Loaded 6126 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): 4792 out of 5149 total matches.
Matched with Tycho-2 5149 out of 11324 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
Forced-photometry filter: calibrated wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits -> calib.txt_param_ref_wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits (aperture=6.0)
Read 11315 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 46.6517 to 64.2527 deg, Dec +16.5180 to +27.2932 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 46.6517 to 64.2527 deg, Dec 16.5180 to 27.2932 deg
Loaded 6135 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): 4773 out of 5143 total matches.
Matched with Tycho-2 5143 out of 11315 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
Forced-photometry filter: calibrated wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits -> calib.txt_param_ref_wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits (aperture=6.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
2.0 pix Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
2.3 pix fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits
2.2 pix fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits
Limiting magnitude estimates:
15.4 mag. Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
15.4 mag. Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
12.7 mag. fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits
12.7 mag. fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits
All-image limiting magnitude estimate: 12.7 (SNR ) 10.3 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.ZIi1Of5a3d (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.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-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits' -> 'wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.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-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
WCS_IMAGE_NAME=wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
WCS-calibrated image found: wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
Checking if the catalog wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.wcscat corresponding to the image wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits alredy exist and is non-empty...
Catalog wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.wcscat corresponding to the image wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
WCS catalog name: wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=882, bad_region=2358, passed=11324
Got 11324 stars (including 8232 good ones) from the SExtractor catalog wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.wcscat
util/solve_plate_with_UCAC5 got 11324 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 4937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4926 matched stars entering correct_measured_positions(), 4926 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4926 matched stars entering correct_measured_positions(), 9434 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
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 4938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4928 matched stars entering correct_measured_positions(), 9434 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4928 matched stars entering correct_measured_positions(), 9434 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 4928 stars left (next iteration limit 5418)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits N_match=4928 sigma_overall_arcsec=0.304 sigma_q1_arcsec=0.383 sigma_q2_arcsec=0.275 sigma_q3_arcsec=0.276 sigma_q4_arcsec=0.235 n_q1=1932 n_q2=884 n_q3=1338 n_q4=774 worst_quadrant_to_overall_ratio=1.262
The image catalog is written to wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits -region wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.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.tQFoSpDJ5m (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.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-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits' -> 'wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.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-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
WCS_IMAGE_NAME=wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
WCS-calibrated image found: wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
Checking if the catalog wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits.wcscat corresponding to the image wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits alredy exist and is non-empty...
Catalog wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits.wcscat corresponding to the image wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
WCS catalog name: wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=893, bad_region=2356, passed=11315
Got 11315 stars (including 8229 good ones) from the SExtractor catalog wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits.wcscat
util/solve_plate_with_UCAC5 got 11315 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 4937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4925 matched stars entering correct_measured_positions(), 4925 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4925 matched stars entering correct_measured_positions(), 9430 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 4938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4927 matched stars entering correct_measured_positions(), 9430 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4927 matched stars entering correct_measured_positions(), 9430 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4927 stars left (next iteration limit 5417)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits N_match=4927 sigma_overall_arcsec=0.327 sigma_q1_arcsec=0.419 sigma_q2_arcsec=0.303 sigma_q3_arcsec=0.295 sigma_q4_arcsec=0.248 n_q1=1928 n_q2=891 n_q3=1332 n_q4=776 worst_quadrant_to_overall_ratio=1.282
The image catalog is written to wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits -region wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.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.0SnQTv0TIo (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_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.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_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits
WCS_IMAGE_NAME=wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits
WCS-calibrated image found: wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits
Checking if the catalog wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits.wcscat corresponding to the image wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits.wcscat corresponding to the image wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits
WCS catalog name: wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=202, bad_region=314, passed=2010
Got 2010 stars (including 1518 good ones) from the SExtractor catalog wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits.wcscat
util/solve_plate_with_UCAC5 got 2010 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.9'
Seting catalog search parameters based on the expected field of view 940.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013068 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010454 (37.6 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 1483 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1482 matched stars entering correct_measured_positions(), 1482 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1482 matched stars entering correct_measured_positions(), 1748 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 1483 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1482 matched stars entering correct_measured_positions(), 1748 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Accuracy estimation diagnostic: 1482 matched stars entering correct_measured_positions(), 1748 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 1482 stars left (next iteration limit 1630)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=1482 robust_rms=6.211 arcsec worst_quadrant_rms=7.397 arcsec
SIP_REFIT: SIP order 3 trial: matched=1482 robust_rms=0.659 arcsec worst_quadrant_rms=0.678 arcsec
SIP_REFIT: SIP order 5 trial: matched=1482 robust_rms=0.524 arcsec worst_quadrant_rms=0.547 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=1482 robust_rms_before=1.819 arcsec robust_rms_before_corrected=0.532 arcsec robust_rms_after=0.524 arcsec worst_quadrant_rms_before=0.612 worst_quadrant_rms_after=0.547
verification OK: wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits
verification OK: wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits
Image size: 941.4'x624.5' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 03:41:31.973 +22:00:03.08 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 2010 stars ###
'wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/correct_sextractor_wcs_catalog_usingxy2sky3224980.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 1.819 -> 0.524 arcsec)
WCS_QUALITY_DIAG: file=fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits N_match=1482 sigma_overall_arcsec=0.536 sigma_q1_arcsec=0.529 sigma_q2_arcsec=0.604 sigma_q3_arcsec=0.534 sigma_q4_arcsec=0.508 n_q1=418 n_q2=182 n_q3=504 n_q4=378 worst_quadrant_to_overall_ratio=1.128
The image catalog is written to wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits -region wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.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.3wTgKObUK6 (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_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.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_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits
WCS_IMAGE_NAME=wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits
WCS-calibrated image found: wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits
Checking if the catalog wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits.wcscat corresponding to the image wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits.wcscat corresponding to the image wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits
WCS catalog name: wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=205, bad_region=324, passed=2015
Got 2015 stars (including 1509 good ones) from the SExtractor catalog wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits.wcscat
util/solve_plate_with_UCAC5 got 2015 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.9'
Seting catalog search parameters based on the expected field of view 940.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013068 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010454 (37.6 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 1477 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1476 matched stars entering correct_measured_positions(), 1476 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1476 matched stars entering correct_measured_positions(), 1741 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 532 to 588 (Dec 16.5 to 27.3)
Done reading UCAC5 zone files...
Matched 1476 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1475 matched stars entering correct_measured_positions(), 1741 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 1475 matched stars entering correct_measured_positions(), 1741 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 1475 stars left (next iteration limit 1623)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=1475 robust_rms=6.214 arcsec worst_quadrant_rms=7.655 arcsec
SIP_REFIT: SIP order 3 trial: matched=1475 robust_rms=0.642 arcsec worst_quadrant_rms=0.717 arcsec
SIP_REFIT: SIP order 5 trial: matched=1475 robust_rms=0.515 arcsec worst_quadrant_rms=0.539 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=1475 robust_rms_before=1.779 arcsec robust_rms_before_corrected=0.524 arcsec robust_rms_after=0.515 arcsec worst_quadrant_rms_before=0.591 worst_quadrant_rms_after=0.539
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.591 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits N_match=1475 sigma_overall_arcsec=0.528 sigma_q1_arcsec=0.527 sigma_q2_arcsec=0.584 sigma_q3_arcsec=0.537 sigma_q4_arcsec=0.549 n_q1=429 n_q2=186 n_q3=490 n_q4=370 worst_quadrant_to_overall_ratio=1.105
The image catalog is written to wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits -region wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.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-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits sigma_overall=0.304 worst_q_ratio=1.262
ref2=Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits sigma_overall=0.327 worst_q_ratio=1.282
new1=fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits sigma_overall=0.536 worst_q_ratio=1.128
new2=fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits sigma_overall=0.528 worst_q_ratio=1.105
reference average sigma_overall=0.3155 worst_q_ratio=1.272
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145_astrometric_residuals.png (4928 matched stars from wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146_astrometric_residuals.png (4927 matched stars from wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.29 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364_astrometric_residuals.png (1482 matched stars from wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.43 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365_astrometric_residuals.png (1475 matched stars from wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.47 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits'
Saving fully-calibrated image wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits'
Preparing the HTML report for the field Tau-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Tau-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
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-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits
SExtractor catalog cache: saved Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.cat to cache
SExtractor catalog cache: saved Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.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-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
Creating symlink local_wcs_cache/wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits
Creating symlink local_wcs_cache/wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.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-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits exists and is non-empty
wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits exists and is non-empty
wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits exists and is non-empty
wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits (1st reference image)
verification OK: wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
Image size: 941.4'x626.9' 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: 03:41:33.240 +21:59:53.22 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-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits (1st new image)
verification OK: wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits
Image size: 940.9'x624.4' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 03:41:31.848 +22:00:04.98 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 03:41:33.240 +21:59:53.22
Second-epoch image center 03:41:31.848 +22:00:04.98
Angular distance between the image centers 0.0063 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits (2nd new image)
verification OK: wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits
Image size: 940.9'x624.4' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 03:41:34.409 +22:00:04.90 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 03:41:33.240 +21:59:53.22
Second-epoch image center 03:41:34.409 +22:00:04.90
Angular distance between the image centers 0.0056 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 03:41:31.848 +22:00:04.98
Second-epoch second image center 03:41:34.409 +22:00:04.90
Angular distance between the image centers 0.00989 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-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits &> /tmp/tmp.BcyTQS5ke5
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits &> /tmp/tmp.TbKa2vKXu5
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits &> /tmp/tmp.PBqmxfqBFy
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits &> /tmp/tmp.Orttt3Yqq8
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits
Calibrating the magnitude scale
Found non-empty wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.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-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits and wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.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-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits and wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.wcscat
Found non-empty wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits and wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.wcscat
The reference image (wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits) and catalog (wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.wcscat) found
'wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.wcscat' -> 'wcsmag.cat'
Read 71179 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 46.6568 to 64.2527 deg, Dec +16.4784 to +27.2943 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 46.6568 to 64.2527 deg, Dec 16.4784 to 27.2943 deg
Loaded 6152 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): 4364 out of 5199 total matches.
Matched with Tycho-2 5199 out of 71179 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.816200
a=0.000000 b=1.000000 c=22.816200
From vast_summary.log: estimated ref. image limiting mag.: -7.20
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.62
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.62
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 71179 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 46.6568 to 64.2527 deg, Dec +16.4784 to +27.2943 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 46.6568 to 64.2527 deg, Dec 16.4784 to 27.2943 deg
Loaded 6152 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): 4364 out of 5199 total matches.
Matched with Tycho-2 5199 out of 71179 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
Forced-photometry filter: calibrated wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits -> calib.txt_param_ref_wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits (aperture=4.6)
Read 71492 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 46.6517 to 64.2527 deg, Dec +16.4684 to +27.2933 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 46.6517 to 64.2527 deg, Dec 16.4684 to 27.2933 deg
Loaded 6156 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): 4369 out of 5198 total matches.
Matched with Tycho-2 5198 out of 71492 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
Forced-photometry filter: calibrated wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits -> calib.txt_param_ref_wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits (aperture=4.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 9 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
1.9 pix Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
2.1 pix fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits
2.1 pix fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits
Limiting magnitude estimates:
15.6 mag. Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
15.6 mag. Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
13.1 mag. fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits
13.1 mag. fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits
All-image limiting magnitude estimate: 13.1 (SNR ) 12.8 (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.BcyTQS5ke5 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.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-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits' -> 'wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.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-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
WCS_IMAGE_NAME=wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
WCS-calibrated image found: wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
Checking if the catalog wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.wcscat corresponding to the image wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits alredy exist and is non-empty...
Catalog wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.wcscat corresponding to the image wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits
WCS catalog name: wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=24, blended=4312, bad_region=11991, passed=71155
Got 71155 stars (including 55407 good ones) from the SExtractor catalog wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.wcscat
util/solve_plate_with_UCAC5 got 71155 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 4940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4935 matched stars entering correct_measured_positions(), 4935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4935 matched stars entering correct_measured_positions(), 61742 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
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 4940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4935 matched stars entering correct_measured_positions(), 61742 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4935 matched stars entering correct_measured_positions(), 61742 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 4935 stars left (next iteration limit 5428)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits N_match=4935 sigma_overall_arcsec=0.295 sigma_q1_arcsec=0.372 sigma_q2_arcsec=0.275 sigma_q3_arcsec=0.264 sigma_q4_arcsec=0.229 n_q1=1854 n_q2=887 n_q3=1405 n_q4=789 worst_quadrant_to_overall_ratio=1.262
The image catalog is written to wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits -region wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.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.TbKa2vKXu5 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.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-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits' -> 'wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.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-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
WCS_IMAGE_NAME=wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
WCS-calibrated image found: wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
Checking if the catalog wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits.wcscat corresponding to the image wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits alredy exist and is non-empty...
Catalog wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits.wcscat corresponding to the image wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits
WCS catalog name: wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=4374, bad_region=12029, passed=71479
Got 71479 stars (including 55644 good ones) from the SExtractor catalog wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits.wcscat
util/solve_plate_with_UCAC5 got 71479 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 4939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4930 matched stars entering correct_measured_positions(), 4930 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4930 matched stars entering correct_measured_positions(), 62079 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 4939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4930 matched stars entering correct_measured_positions(), 62079 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4930 matched stars entering correct_measured_positions(), 62079 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 4930 stars left (next iteration limit 5423)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits N_match=4930 sigma_overall_arcsec=0.309 sigma_q1_arcsec=0.396 sigma_q2_arcsec=0.292 sigma_q3_arcsec=0.279 sigma_q4_arcsec=0.240 n_q1=1847 n_q2=888 n_q3=1401 n_q4=794 worst_quadrant_to_overall_ratio=1.281
The image catalog is written to wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits -region wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.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.PBqmxfqBFy (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_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.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_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits
WCS_IMAGE_NAME=wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits
WCS-calibrated image found: wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits
Checking if the catalog wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits.wcscat corresponding to the image wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits.wcscat corresponding to the image wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits
WCS catalog name: wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=372, bad_region=1687, passed=14583
Got 14583 stars (including 12551 good ones) from the SExtractor catalog wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits.wcscat
util/solve_plate_with_UCAC5 got 14583 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.9'
Seting catalog search parameters based on the expected field of view 940.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013068 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010454 (37.6 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 4929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4917 matched stars entering correct_measured_positions(), 4917 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4917 matched stars entering correct_measured_positions(), 13409 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
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 4930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4918 matched stars entering correct_measured_positions(), 13409 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 4918 matched stars entering correct_measured_positions(), 13409 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 4918 stars left (next iteration limit 5408)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits N_match=4918 sigma_overall_arcsec=0.508 sigma_q1_arcsec=0.509 sigma_q2_arcsec=0.566 sigma_q3_arcsec=0.498 sigma_q4_arcsec=0.493 n_q1=1422 n_q2=655 n_q3=1617 n_q4=1224 worst_quadrant_to_overall_ratio=1.115
The image catalog is written to wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits -region wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.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.Orttt3Yqq8 (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_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.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_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits
WCS_IMAGE_NAME=wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits
WCS-calibrated image found: wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits
Checking if the catalog wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits.wcscat corresponding to the image wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits alredy exist and is non-empty...
Catalog wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits.wcscat corresponding to the image wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits
WCS catalog name: wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=408, bad_region=1730, passed=14941
Got 14941 stars (including 12840 good ones) from the SExtractor catalog wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits.wcscat
util/solve_plate_with_UCAC5 got 14941 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 940.9'
Seting catalog search parameters based on the expected field of view 940.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013068 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010454 (37.6 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 4928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4919 matched stars entering correct_measured_positions(), 4920 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4919 matched stars entering correct_measured_positions(), 13747 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
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 4928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4919 matched stars entering correct_measured_positions(), 13747 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 4919 matched stars entering correct_measured_positions(), 13747 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 4919 stars left (next iteration limit 5410)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits is a symbolic link - not rewriting the WCS of whatever it points to, keeping the original solution
WCS_QUALITY_DIAG: file=fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits N_match=4919 sigma_overall_arcsec=0.521 sigma_q1_arcsec=0.517 sigma_q2_arcsec=0.542 sigma_q3_arcsec=0.529 sigma_q4_arcsec=0.514 n_q1=1438 n_q2=658 n_q3=1627 n_q4=1196 worst_quadrant_to_overall_ratio=1.040
The image catalog is written to wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits -region wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.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-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.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_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-13-36_20.00sec_-0.00C_LIGHT_0364.fits
Saving fully-calibrated image wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.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_2026-07-30_CI_Tau-02-Q2b1x1_044602_TTUQ2b1x1_3216708_mOkZzdxQ/wcs_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365.fits
Preparing the HTML report for the field Tau-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:43:55.82 +22:36:35.6: 16.32 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:50:40.92 +23:42:09.2: 16.26 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:46:09.89 +23:08:08.1: 12.84 +/- 0.02 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:34:11.24 +21:22:02.8: 12.81 +/- 0.02 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-15-49_20.00sec_-14.90C_LIGHT_0145.fits at 03:43:21.20 +18:01:20.9: 13.09 +/- 0.02 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:46:09.89 +23:08:08.1: 12.87 +/- 0.02 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:50:40.92 +23:42:09.2: 16.29 +/- 99.00 upperlimit
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:34:11.24 +21:22:02.8: 12.85 +/- 0.02 detection
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:43:55.82 +22:36:35.6: 16.30 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 12.85 +/- 0.01
Forced photometry reference-image weighted average: 12.83 +/- 0.01
Forced photometry filter REJECTED candidate at 03:46:09.89 +23:08:08.1: ref_mag=12.85 +/- 0.01 new_mean_mag=12.6745 delta=0.18 (need > 0.90)
Forced photometry filter REJECTED candidate at 03:34:11.24 +21:22:02.8: ref_mag=12.83 +/- 0.01 new_mean_mag=12.7527 delta=0.08 (need > 0.90)
Forced photometry on wcs_Tau-02-Q2b1x1_2026-01-08_22-16-30_20.00sec_-15.00C_LIGHT_0146.fits at 03:43:21.20 +18:01:20.9: 13.15 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.01
Forced photometry filter KEPT candidate at 03:43:21.20 +18:01:20.9: ref_mag=13.12 +/- 0.01 new_mean_mag=12.2003 delta=0.92 (need > 0.90)
Adding exclusion_list_local.txt__out57655.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out87594.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out88483.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 4s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 86036_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365
The candidate 86036_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365 did not pass the final checks
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Considering the candidate 87391_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365
The candidate 87391_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365 did not pass the final checks
**** FOUND 03:53:04.36 +25:32:36.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 87594_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365
Preparing report for the candidate 87594_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365
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Considering the candidate 87935_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365
The candidate 87935_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365 did not pass the final checks
**** FOUND 03:48:54.42 +23:50:01.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 88318_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365
The candidate 88318_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365 did not pass the final checks
**** FOUND 03:31:40.64 +18:47:35.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 88483_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365
Preparing report for the candidate 88483_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365
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Considering the candidate 88512_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365
The candidate 88512_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365 did not pass the final checks
**** FOUND 03:49:07.50 +24:00:40.3 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 88779_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365
The candidate 88779_fd_Tau-02-Q2b1x1_2026-07-30_03-14-17_20.00sec_-0.00C_LIGHT_0365 did not pass the final checks