This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 08 22.4017 2461274.9017 12.54 01:41:20.04 -22:48:57.3
194.78072 -77.90562 galactic Cet Second-epoch detections are separated by 1.9" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 01:41:20.04 -22:48:57.3 (user input) | T | P | (position from user input) J-Ks=0.430+/-0.034 (G)
Forced photometry on wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:41:20.04 -22:48:57.3: 13.98 +/- 0.36 detection
Forced photometry on wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:41:20.04 -22:48:57.3: 13.54 +/- 0.26 detection
Forced photometry reference-image weighted average: 13.69 +/- 0.21
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 08 22.4017* 01 41 20.04 -22 48 57.3 12.5 U Cet 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
target,2461274.9017,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260822.4017 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 08 22.4017 2461274.9017 12.38 01:43:23.17 -22:54:12.4
196.02424 -77.50431 galactic Cet Second-epoch detections are separated by 1.1" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | DocumentRef: VOTx3528651 | 01:43:23.17 -22:54:12.4 (user input) | (VSX @ VizieR) | (VSX @ VizieR) | (position from user input) J-Ks=0.379+/-0.035 (G)
Forced photometry on wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:43:23.17 -22:54:12.4: 13.23 +/- 0.18 detection
Forced photometry on wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:43:23.17 -22:54:12.4: 13.37 +/- 0.23 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.14
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 08 22.4017* 01 43 23.17 -22 54 12.4 12.4 U Cet 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
DocumentRef: VOTx3528651,2461274.9017,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
DocumentRef: VOTx3528651 20260822.4017 12.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461242.96007139 21.07.2026 11:02:20.168 /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
First image: 2461242.96007139 21.07.2026 11:02:20.168 /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
Last image: 2461274.90202270 22.08.2026 09:38:44.761 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -9.35
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): 1318
Objects passed selection criteria: 1317
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 1198.25
Average stars matched: 1188 (99.1446 %)
Memory usage VmPeak: 228432 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Aug 20 15:05:04 CDT 2026
VaST build number 1.0rc89-192-g23359006
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-20)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Aug 22 04:43:54 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: 2461242.96007139 21.07.2026 11:02:20.168 /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
First image: 2461242.96007139 21.07.2026 11:02:20.168 /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
Last image: 2461274.90202270 22.08.2026 09:38:44.761 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 15
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -9.12
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 5 seconds
Number of parallel threads: 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): 7782
Objects passed selection criteria: 7775
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 7207
Average stars matched: 7049.5 (97.8146 %)
Memory usage VmPeak: 234072 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Aug 20 15:05:04 CDT 2026
VaST build number 1.0rc89-192-g23359006
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-20)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Aug 22 04:44:30 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits
SExtractor catalog cache: saved For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits.cat to cache
SExtractor catalog cache: saved For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.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/For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.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: 2461274.90146294
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_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits exists and is non-empty
wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits exists and is non-empty
wcs_fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits exists and is non-empty
wcs_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits (1st reference image)
verification OK: wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
Image size: 941.4'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:55:22.664 -26:00:04.01 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_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits (1st new image)
verification OK: wcs_fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits
Image size: 940.9'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: 01:55:08.329 -26:02:26.37 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 01:55:22.664 -26:00:04.01
Second-epoch image center 01:55:08.329 -26:02:26.37
Angular distance between the image centers 0.0667 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits (2nd new image)
verification OK: wcs_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits
Image size: 940.9'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:55:05.544 -26:02:24.39 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:55:22.664 -26:00:04.01
Second-epoch image center 01:55:05.544 -26:02:24.39
Angular distance between the image centers 0.0750 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 01:55:08.329 -26:02:26.37
Second-epoch second image center 01:55:05.544 -26:02:24.39
Angular distance between the image centers 0.01044 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/For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits &> /tmp/tmp.ykWaGcp0Qh
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits &> /tmp/tmp.PxaEIa8Dsy
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits &> /tmp/tmp.hnW32i8vhC
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits &> /tmp/tmp.9c0Tev8Ygo
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits
Calibrating the magnitude scale
Found non-empty wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.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_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits and wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.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_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits and wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits.wcscat
Found non-empty wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits and wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits.wcscat
The reference image (wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits) and catalog (wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits.wcscat) found
'wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits.wcscat' -> 'wcsmag.cat'
Read 1410 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 19.5210 to 37.6556 deg, Dec -31.4428 to -20.2852 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 19.5210 to 37.6556 deg, Dec -31.4428 to -20.2852 deg
Loaded 4541 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): 1056 out of 1077 total matches.
Matched with Tycho-2 1077 out of 1410 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.598350
a=0.000000 b=1.000000 c=22.598350
From vast_summary.log: estimated ref. image limiting mag.: -9.35
Updating vast_summary.log: Estimated ref. image limiting mag.: 13.25
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 13.25
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 1410 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 19.5210 to 37.6556 deg, Dec -31.4428 to -20.2852 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 19.5210 to 37.6556 deg, Dec -31.4428 to -20.2852 deg
Loaded 4541 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): 1056 out of 1077 total matches.
Matched with Tycho-2 1077 out of 1410 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
Forced-photometry filter: calibrated wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits -> calib.txt_param_ref_wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits (aperture=6.5)
Read 1319 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 19.5208 to 37.6551 deg, Dec -31.4009 to -20.2852 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 19.5208 to 37.6551 deg, Dec -31.4009 to -20.2852 deg
Loaded 4524 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): 969 out of 996 total matches.
Matched with Tycho-2 996 out of 1319 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
Forced-photometry filter: calibrated wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits -> calib.txt_param_ref_wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits (aperture=6.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.8 pix For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
2.7 pix For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
2.9 pix fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits
2.9 pix fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits
Limiting magnitude estimates:
13.3 mag. For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
13.2 mag. For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
12.1 mag. fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits
12.1 mag. fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits
All-image limiting magnitude estimate: 12.1 (SNR ) 10.1 (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
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.ykWaGcp0Qh (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits' -> 'wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.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/For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
WCS_IMAGE_NAME=wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
WCS-calibrated image found: wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
Checking if the catalog wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits.wcscat corresponding to the image wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits alredy exist and is non-empty...
Catalog wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits.wcscat corresponding to the image wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
WCS catalog name: wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=215, bad_region=0, passed=1410
Got 1410 stars (including 1194 good ones) from the SExtractor catalog wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits.wcscat
util/solve_plate_with_UCAC5 got 1410 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 292 to 350 (Dec -31.4 to -20.3)
Done reading UCAC5 zone files...
Matched 1174 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1174 matched stars entering correct_measured_positions(), 1164 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1174 matched stars entering correct_measured_positions(), 1396 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 292 to 350 (Dec -31.4 to -20.3)
Done reading UCAC5 zone files...
Matched 1173 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1173 matched stars entering correct_measured_positions(), 1396 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 1173 matched stars entering correct_measured_positions(), 1396 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 1173 stars left (next iteration limit 1291)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits N_match=1173 sigma_overall_arcsec=0.303 sigma_q1_arcsec=0.305 sigma_q2_arcsec=0.311 sigma_q3_arcsec=0.299 sigma_q4_arcsec=0.278 n_q1=303 n_q2=311 n_q3=280 n_q4=279 worst_quadrant_to_overall_ratio=1.025
The image catalog is written to wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits -region wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.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.PxaEIa8Dsy (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits' -> 'wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.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/For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
WCS_IMAGE_NAME=wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
WCS-calibrated image found: wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
Checking if the catalog wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits.wcscat corresponding to the image wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits alredy exist and is non-empty...
Catalog wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits.wcscat corresponding to the image wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
WCS catalog name: wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=225, bad_region=0, passed=1319
Got 1319 stars (including 1094 good ones) from the SExtractor catalog wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits.wcscat
util/solve_plate_with_UCAC5 got 1319 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 292 to 350 (Dec -31.4 to -20.3)
Done reading UCAC5 zone files...
Matched 1076 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1076 matched stars entering correct_measured_positions(), 1063 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1076 matched stars entering correct_measured_positions(), 1301 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 292 to 350 (Dec -31.4 to -20.3)
Done reading UCAC5 zone files...
Matched 1076 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1076 matched stars entering correct_measured_positions(), 1300 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 1076 matched stars entering correct_measured_positions(), 1300 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 1076 stars left (next iteration limit 1183)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits N_match=1076 sigma_overall_arcsec=0.316 sigma_q1_arcsec=0.372 sigma_q2_arcsec=0.336 sigma_q3_arcsec=0.269 sigma_q4_arcsec=0.302 n_q1=277 n_q2=289 n_q3=262 n_q4=248 worst_quadrant_to_overall_ratio=1.176
The image catalog is written to wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits -region wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.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.hnW32i8vhC (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits
WCS_IMAGE_NAME=wcs_fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits
WCS-calibrated image found: wcs_fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits
Checking if the catalog wcs_fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits.wcscat corresponding to the image wcs_fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits alredy exist and is non-empty...
Catalog wcs_fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits.wcscat corresponding to the image wcs_fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits
WCS catalog name: wcs_fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=67, bad_region=0, passed=1036
Got 1036 stars (including 967 good ones) from the SExtractor catalog wcs_fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits.wcscat
util/solve_plate_with_UCAC5 got 1036 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 292 to 350 (Dec -31.5 to -20.3)
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 931 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 1007 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 350 (Dec -31.5 to -20.3)
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 1008 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 948 matched stars entering correct_measured_positions(), 1008 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 948 stars left (next iteration limit 1042)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=948 robust_rms=8.051 arcsec worst_quadrant_rms=12.616 arcsec
SIP_REFIT: SIP order 3 trial: matched=948 robust_rms=0.408 arcsec worst_quadrant_rms=0.467 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=948 robust_rms_before=0.918 arcsec robust_rms_before_corrected=0.346 arcsec robust_rms_after=0.408 arcsec worst_quadrant_rms_before=0.414 worst_quadrant_rms_after=0.467
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.414 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits N_match=948 sigma_overall_arcsec=0.354 sigma_q1_arcsec=0.429 sigma_q2_arcsec=0.389 sigma_q3_arcsec=0.315 sigma_q4_arcsec=0.310 n_q1=246 n_q2=200 n_q3=291 n_q4=211 worst_quadrant_to_overall_ratio=1.211
The image catalog is written to wcs_fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits -region wcs_fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.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.9c0Tev8Ygo (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits
WCS_IMAGE_NAME=wcs_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits
WCS-calibrated image found: wcs_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits
Checking if the catalog wcs_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits.wcscat corresponding to the image wcs_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits alredy exist and is non-empty...
Catalog wcs_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits.wcscat corresponding to the image wcs_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits
WCS catalog name: wcs_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=62, bad_region=0, passed=1059
Got 1059 stars (including 996 good ones) from the SExtractor catalog wcs_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits.wcscat
util/solve_plate_with_UCAC5 got 1059 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 292 to 350 (Dec -31.5 to -20.3)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 960 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 1034 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 350 (Dec -31.5 to -20.3)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 1032 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 1032 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=976 robust_rms=7.984 arcsec worst_quadrant_rms=13.193 arcsec
SIP_REFIT: SIP order 3 trial: matched=976 robust_rms=0.426 arcsec worst_quadrant_rms=0.467 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=976 robust_rms_before=0.932 arcsec robust_rms_before_corrected=0.351 arcsec robust_rms_after=0.426 arcsec worst_quadrant_rms_before=0.412 worst_quadrant_rms_after=0.467
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.412 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits N_match=976 sigma_overall_arcsec=0.362 sigma_q1_arcsec=0.417 sigma_q2_arcsec=0.425 sigma_q3_arcsec=0.331 sigma_q4_arcsec=0.307 n_q1=252 n_q2=203 n_q3=300 n_q4=221 worst_quadrant_to_overall_ratio=1.172
The image catalog is written to wcs_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits -region wcs_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Saving the final (post-refit) wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits to local_wcs_cache/
'wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits' -> 'local_wcs_cache/wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits'
Saving the final (post-refit) wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits to local_wcs_cache/
'wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits' -> 'local_wcs_cache/wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits'
Saving the final (post-refit) wcs_fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits to local_wcs_cache/
'wcs_fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits' -> 'local_wcs_cache/wcs_fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits'
Saving the final (post-refit) wcs_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits to local_wcs_cache/
'wcs_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits' -> 'local_wcs_cache/wcs_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits sigma_overall=0.303 worst_q_ratio=1.025
ref2=For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits sigma_overall=0.316 worst_q_ratio=1.176
new1=fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits sigma_overall=0.354 worst_q_ratio=1.211
new2=fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits sigma_overall=0.362 worst_q_ratio=1.172
reference average sigma_overall=0.3095 worst_q_ratio=1.1005
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897_astrometric_residuals.png (1173 matched stars from wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.29 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898_astrometric_residuals.png (1076 matched stars from wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138_astrometric_residuals.png (948 matched stars from wcs_fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.33 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139_astrometric_residuals.png (976 matched stars from wcs_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.33 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/wcs_fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits'
Saving fully-calibrated image wcs_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/wcs_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits'
Preparing the HTML report for the field For-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:36:33.17 -25:22:06.2: 10.59 +/- 0.02 detection
Forced photometry on wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:34:42.38 -23:26:16.9: 10.75 +/- 0.02 detection
Forced photometry on wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:36:33.17 -25:22:06.2: 10.59 +/- 0.02 detection
Forced photometry on wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:34:42.38 -23:26:16.9: 10.80 +/- 0.02 detection
Forced photometry reference-image weighted average: 10.59 +/- 0.01
Forced photometry reference-image weighted average: 10.77 +/- 0.02
Forced photometry filter REJECTED candidate at 01:36:33.17 -25:22:06.2: ref_mag=10.59 +/- 0.01 new_mean_mag=10.1937 delta=0.40 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:34:42.38 -23:26:16.9: ref_mag=10.77 +/- 0.02 new_mean_mag=10.3185 delta=0.46 (need > 0.90)
make_report_in_HTML.sh Phase 1 (network queries): 1s
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: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20029_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139
The candidate 20029_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20032_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139
The candidate 20032_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139 did not pass the final checks
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field For-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits
SExtractor catalog cache: saved For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits.cat to cache
SExtractor catalog cache: saved For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
Creating symlink local_wcs_cache/wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
Creating symlink local_wcs_cache/wcs_fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits
Creating symlink local_wcs_cache/wcs_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits
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_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits exists and is non-empty
wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits exists and is non-empty
wcs_fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits exists and is non-empty
wcs_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits (1st reference image)
verification OK: wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
Image size: 941.4'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:55:22.664 -26:00:04.01 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_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits (1st new image)
verification OK: wcs_fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits
Image size: 940.9'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: 01:55:08.329 -26:02:26.37 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 01:55:22.664 -26:00:04.01
Second-epoch image center 01:55:08.329 -26:02:26.37
Angular distance between the image centers 0.0667 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits (2nd new image)
verification OK: wcs_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits
Image size: 940.9'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 01:55:05.544 -26:02:24.39 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 01:55:22.664 -26:00:04.01
Second-epoch image center 01:55:05.544 -26:02:24.39
Angular distance between the image centers 0.0750 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 01:55:08.329 -26:02:26.37
Second-epoch second image center 01:55:05.544 -26:02:24.39
Angular distance between the image centers 0.01044 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/For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits &> /tmp/tmp.c78VHMuzJ9
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits &> /tmp/tmp.953oOzEZWd
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits &> /tmp/tmp.FUC7dNiGTp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits &> /tmp/tmp.jo1jAEzqTE
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits
Calibrating the magnitude scale
Found non-empty wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.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_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits and wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.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_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits and wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits.wcscat
Found non-empty wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits and wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits.wcscat
The reference image (wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits) and catalog (wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits.wcscat) found
'wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits.wcscat' -> 'wcsmag.cat'
Read 8445 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 19.4281 to 37.6591 deg, Dec -31.4428 to -20.1306 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 19.4281 to 37.6591 deg, Dec -31.4428 to -20.1306 deg
Loaded 4632 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): 3537 out of 3586 total matches.
Matched with Tycho-2 3586 out of 8445 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.479400
a=0.000000 b=1.000000 c=22.479400
From vast_summary.log: estimated ref. image limiting mag.: -9.12
Updating vast_summary.log: Estimated ref. image limiting mag.: 13.36
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 13.36
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 8445 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 19.4281 to 37.6591 deg, Dec -31.4428 to -20.1306 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 19.4281 to 37.6591 deg, Dec -31.4428 to -20.1306 deg
Loaded 4632 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): 3537 out of 3586 total matches.
Matched with Tycho-2 3586 out of 8445 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
Forced-photometry filter: calibrated wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits -> calib.txt_param_ref_wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits (aperture=5.3)
Read 7913 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 19.4274 to 37.6551 deg, Dec -31.4418 to -20.1302 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 19.4274 to 37.6551 deg, Dec -31.4418 to -20.1302 deg
Loaded 4630 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): 3535 out of 3585 total matches.
Matched with Tycho-2 3585 out of 7913 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
Forced-photometry filter: calibrated wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits -> calib.txt_param_ref_wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits (aperture=5.3)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 14 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.5 pix For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
2.5 pix For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
2.7 pix fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits
2.7 pix fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits
Limiting magnitude estimates:
13.4 mag. For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
13.3 mag. For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
12.6 mag. fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits
12.6 mag. fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits
All-image limiting magnitude estimate: 12.6 (SNR ) 12.2 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.c78VHMuzJ9 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits' -> 'wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.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/For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
WCS_IMAGE_NAME=wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
WCS-calibrated image found: wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
Checking if the catalog wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits.wcscat corresponding to the image wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits alredy exist and is non-empty...
Catalog wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits.wcscat corresponding to the image wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits
WCS catalog name: wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=258, bad_region=0, passed=8444
Got 8444 stars (including 8174 good ones) from the SExtractor catalog wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits.wcscat
util/solve_plate_with_UCAC5 got 8444 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 292 to 351 (Dec -31.4 to -20.1)
Done reading UCAC5 zone files...
Matched 4889 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4887 matched stars entering correct_measured_positions(), 4887 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4887 matched stars entering correct_measured_positions(), 8444 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.4 to -20.1)
Done reading UCAC5 zone files...
Matched 4889 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4887 matched stars entering correct_measured_positions(), 8444 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 4887 matched stars entering correct_measured_positions(), 8444 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 4887 stars left (next iteration limit 5375)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits N_match=4887 sigma_overall_arcsec=0.513 sigma_q1_arcsec=0.591 sigma_q2_arcsec=0.615 sigma_q3_arcsec=0.424 sigma_q4_arcsec=0.453 n_q1=1218 n_q2=1175 n_q3=1226 n_q4=1268 worst_quadrant_to_overall_ratio=1.197
The image catalog is written to wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits -region wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.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.953oOzEZWd (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits' -> 'wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.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/For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
WCS_IMAGE_NAME=wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
WCS-calibrated image found: wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
Checking if the catalog wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits.wcscat corresponding to the image wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits alredy exist and is non-empty...
Catalog wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits.wcscat corresponding to the image wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits
WCS catalog name: wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=250, bad_region=0, passed=7912
Got 7912 stars (including 7654 good ones) from the SExtractor catalog wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits.wcscat
util/solve_plate_with_UCAC5 got 7912 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 292 to 351 (Dec -31.4 to -20.1)
Done reading UCAC5 zone files...
Matched 4895 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4892 matched stars entering correct_measured_positions(), 4892 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4892 matched stars entering correct_measured_positions(), 7912 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.4 to -20.1)
Done reading UCAC5 zone files...
Matched 4895 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4892 matched stars entering correct_measured_positions(), 7912 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Accuracy estimation diagnostic: 4892 matched stars entering correct_measured_positions(), 7912 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.56"
Excluding outliers - 4892 stars left (next iteration limit 5381)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits N_match=4892 sigma_overall_arcsec=0.541 sigma_q1_arcsec=0.642 sigma_q2_arcsec=0.623 sigma_q3_arcsec=0.466 sigma_q4_arcsec=0.467 n_q1=1217 n_q2=1178 n_q3=1222 n_q4=1275 worst_quadrant_to_overall_ratio=1.186
The image catalog is written to wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits -region wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.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.FUC7dNiGTp (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits
WCS_IMAGE_NAME=wcs_fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits
WCS-calibrated image found: wcs_fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits
Checking if the catalog wcs_fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits.wcscat corresponding to the image wcs_fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits alredy exist and is non-empty...
Catalog wcs_fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits.wcscat corresponding to the image wcs_fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits
WCS catalog name: wcs_fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=118, bad_region=1, passed=6253
Got 6253 stars (including 6126 good ones) from the SExtractor catalog wcs_fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits.wcscat
util/solve_plate_with_UCAC5 got 6253 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 292 to 351 (Dec -31.5 to -20.2)
Done reading UCAC5 zone files...
Matched 4869 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4865 matched stars entering correct_measured_positions(), 4865 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4865 matched stars entering correct_measured_positions(), 6253 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.5 to -20.2)
Done reading UCAC5 zone files...
Matched 4869 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4865 matched stars entering correct_measured_positions(), 6253 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
Accuracy estimation diagnostic: 4865 matched stars entering correct_measured_positions(), 6253 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
Excluding outliers - 4865 stars left (next iteration limit 5351)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4865 robust_rms=8.051 arcsec worst_quadrant_rms=10.622 arcsec
SIP_REFIT: SIP order 3 trial: matched=4865 robust_rms=0.809 arcsec worst_quadrant_rms=1.036 arcsec
SIP_REFIT: SIP order 5 trial: matched=4865 robust_rms=0.754 arcsec worst_quadrant_rms=0.949 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4865 robust_rms_before=1.174 arcsec robust_rms_before_corrected=0.763 arcsec robust_rms_after=0.754 arcsec worst_quadrant_rms_before=0.965 worst_quadrant_rms_after=0.949
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.965 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits N_match=4865 sigma_overall_arcsec=0.680 sigma_q1_arcsec=0.854 sigma_q2_arcsec=0.825 sigma_q3_arcsec=0.574 sigma_q4_arcsec=0.613 n_q1=1174 n_q2=896 n_q3=1494 n_q4=1301 worst_quadrant_to_overall_ratio=1.257
The image catalog is written to wcs_fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits -region wcs_fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.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.jo1jAEzqTE (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits
WCS_IMAGE_NAME=wcs_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits
WCS-calibrated image found: wcs_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits
Checking if the catalog wcs_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits.wcscat corresponding to the image wcs_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits alredy exist and is non-empty...
Catalog wcs_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits.wcscat corresponding to the image wcs_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits
WCS catalog name: wcs_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=112, bad_region=1, passed=6381
Got 6381 stars (including 6262 good ones) from the SExtractor catalog wcs_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits.wcscat
util/solve_plate_with_UCAC5 got 6381 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 292 to 351 (Dec -31.5 to -20.2)
Done reading UCAC5 zone files...
Matched 4874 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4871 matched stars entering correct_measured_positions(), 4871 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4871 matched stars entering correct_measured_positions(), 6381 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 292 to 351 (Dec -31.5 to -20.2)
Done reading UCAC5 zone files...
Matched 4874 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4871 matched stars entering correct_measured_positions(), 6381 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Accuracy estimation diagnostic: 4871 matched stars entering correct_measured_positions(), 6381 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Excluding outliers - 4871 stars left (next iteration limit 5358)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4871 robust_rms=8.456 arcsec worst_quadrant_rms=11.258 arcsec
SIP_REFIT: SIP order 3 trial: matched=4871 robust_rms=0.831 arcsec worst_quadrant_rms=1.052 arcsec
SIP_REFIT: SIP order 5 trial: matched=4871 robust_rms=0.734 arcsec worst_quadrant_rms=0.973 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4871 robust_rms_before=1.173 arcsec robust_rms_before_corrected=0.750 arcsec robust_rms_after=0.734 arcsec worst_quadrant_rms_before=0.961 worst_quadrant_rms_after=0.973
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.961 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits N_match=4871 sigma_overall_arcsec=0.675 sigma_q1_arcsec=0.851 sigma_q2_arcsec=0.847 sigma_q3_arcsec=0.581 sigma_q4_arcsec=0.570 n_q1=1173 n_q2=913 n_q3=1480 n_q4=1305 worst_quadrant_to_overall_ratio=1.262
The image catalog is written to wcs_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits -region wcs_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.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_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/wcs_fd_For-01-Q1b1x1_2026-08-22_04-37-56_20.00sec_-0.00C_LIGHTs_0138.fits
Saving fully-calibrated image wcs_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-08-22_CI_For-01-Q1b1x1_043952_TTUQ1b1x1_3071501_9jxoXcIA/wcs_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139.fits
Preparing the HTML report for the field For-01-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:37:36.82 -25:29:51.8: 13.02 +/- 0.14 detection
Forced photometry on wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 02:01:52.17 -27:00:32.4: 13.43 +/- 0.20 detection
Forced photometry on wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:34:36.89 -21:03:17.4: 12.83 +/- 0.14 detection
Forced photometry on wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:43:23.17 -22:54:12.4: 13.23 +/- 0.18 detection
Forced photometry on wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:31:59.94 -24:55:38.9: 13.35 +/- 0.21 detection
Forced photometry on wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:38:01.35 -23:17:34.3: 13.46 +/- 0.23 detection
Forced photometry on wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:41:20.04 -22:48:57.3: 13.98 +/- 0.36 detection
Forced photometry on wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:41:09.95 -23:13:11.1: 13.28 +/- 0.19 detection
Forced photometry on wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:59:05.95 -23:27:45.9: 13.15 +/- 0.16 detection
Forced photometry on wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:40:57.44 -23:42:40.4: 13.38 +/- 0.20 detection
Forced photometry on wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:40:57.44 -23:42:40.4: 13.56 +/- 0.27 detection
Forced photometry on wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:41:20.04 -22:48:57.3: 13.54 +/- 0.26 detection
Forced photometry on wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 02:01:52.17 -27:00:32.4: 13.27 +/- 0.18 detection
Forced photometry on wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:34:36.89 -21:03:17.4: 12.89 +/- 0.16 detection
Forced photometry on wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:59:05.95 -23:27:45.9: 13.73 +/- 0.29 detection
Forced photometry on wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:37:36.82 -25:29:51.8: 13.51 +/- 0.25 detection
Forced photometry on wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:31:59.94 -24:55:38.9: 13.13 +/- 0.19 detection
Forced photometry on wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:43:23.17 -22:54:12.4: 13.37 +/- 0.23 detection
Forced photometry on wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:38:01.35 -23:17:34.3: 13.16 +/- 0.18 detection
Forced photometry on wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:41:09.95 -23:13:11.1: 13.49 +/- 0.25 detection
Forced photometry reference-image weighted average: 13.44 +/- 0.16
Forced photometry reference-image weighted average: 13.69 +/- 0.21
Forced photometry reference-image weighted average: 13.29 +/- 0.14
Forced photometry reference-image weighted average: 13.34 +/- 0.14
Forced photometry reference-image weighted average: 12.86 +/- 0.11
Forced photometry reference-image weighted average: 13.29 +/- 0.14
Forced photometry reference-image weighted average: 13.22 +/- 0.14
Forced photometry reference-image weighted average: 13.14 +/- 0.12
Forced photometry reference-image weighted average: 13.27 +/- 0.14
Forced photometry filter KEPT candidate at 01:40:57.44 -23:42:40.4: ref_mag=13.44 +/- 0.16 new_mean_mag=12.5195 delta=0.92 (need > 0.90)
Forced photometry reference-image weighted average: 13.35 +/- 0.15
Forced photometry filter KEPT candidate at 01:41:20.04 -22:48:57.3: ref_mag=13.69 +/- 0.21 new_mean_mag=12.5120 delta=1.18 (need > 0.90)
Forced photometry filter REJECTED candidate at 02:01:52.17 -27:00:32.4: ref_mag=13.34 +/- 0.14 new_mean_mag=12.5128 delta=0.83 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:59:05.95 -23:27:45.9: ref_mag=13.29 +/- 0.14 new_mean_mag=12.3882 delta=0.90 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:34:36.89 -21:03:17.4: ref_mag=12.86 +/- 0.11 new_mean_mag=12.4539 delta=0.41 (need > 0.90)
Forced photometry filter KEPT candidate at 01:43:23.17 -22:54:12.4: ref_mag=13.29 +/- 0.14 new_mean_mag=12.3589 delta=0.93 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:38:01.35 -23:17:34.3: ref_mag=13.27 +/- 0.14 new_mean_mag=12.4608 delta=0.81 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:37:36.82 -25:29:51.8: ref_mag=13.14 +/- 0.12 new_mean_mag=12.2990 delta=0.84 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:31:59.94 -24:55:38.9: ref_mag=13.22 +/- 0.14 new_mean_mag=12.4692 delta=0.75 (need > 0.90)
Forced photometry filter REJECTED candidate at 01:41:09.95 -23:13:11.1: ref_mag=13.35 +/- 0.15 new_mean_mag=12.4554 delta=0.90 (need > 0.90)
Forced photometry on wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:42:44.85 -22:52:34.1: 13.53 +/- 0.24 detection
Forced photometry on wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:40:14.72 -22:06:42.8: 13.71 +/- 0.30 detection
Forced photometry on wcs_For-01-Q1b1x1_2026-07-21_06-02-20_20.00sec_0.00C_LIGHTs_0897.fits at 01:47:01.38 -22:41:41.5: 13.48 +/- 0.22 detection
Forced photometry on wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:40:14.72 -22:06:42.8: 13.25 +/- 0.21 detection
Forced photometry on wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:42:44.85 -22:52:34.1: 13.92 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.39 +/- 0.17
Forced photometry filter REJECTED candidate at 01:40:14.72 -22:06:42.8: ref_mag=13.39 +/- 0.17 new_mean_mag=12.5991 delta=0.79 (need > 0.90)
Forced photometry reference-image weighted average: 13.53 +/- 0.24
Forced photometry filter KEPT candidate at 01:42:44.85 -22:52:34.1: ref_mag=13.53 +/- 0.24 new_mean_mag=12.5158 delta=1.02 (need > 0.90)
Forced photometry on wcs_For-01-Q1b1x1_2026-07-21_06-03-20_20.00sec_-0.00C_LIGHTs_0898.fits at 01:47:01.38 -22:41:41.5: 13.31 +/- 0.20 detection
Forced photometry reference-image weighted average: 13.39 +/- 0.15
Forced photometry filter REJECTED candidate at 01:47:01.38 -22:41:41.5: ref_mag=13.39 +/- 0.15 new_mean_mag=12.6253 delta=0.76 (need > 0.90)
Adding exclusion_list_gaiadr2.txt__out20464.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out20491.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out20457.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20462.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 163s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 20439_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139
The candidate 20439_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139 did not pass the final checks
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Considering the candidate 20442_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139
The candidate 20442_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139 did not pass the final checks
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Considering the candidate 20448_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139
The candidate 20448_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139 did not pass the final checks
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Considering the candidate 20454_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139
The candidate 20454_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139 did not pass the final checks
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Considering the candidate 20457_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139
Preparing report for the candidate 20457_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139
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Considering the candidate 20458_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139
The candidate 20458_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139 did not pass the final checks
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Considering the candidate 20460_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139
The candidate 20460_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139 did not pass the final checks
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Considering the candidate 20461_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139
The candidate 20461_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139 did not pass the final checks
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Considering the candidate 20462_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139
Preparing report for the candidate 20462_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139
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Considering the candidate 20464_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139
The candidate 20464_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139 did not pass the final checks
**** FOUND 01:40:57.44 -23:42:40.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)GAIADR2_OUTPUT=# 1.204 5039090416055383424 025.23902782888 -23.71140539437 13.5002 13.1059 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.204#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 20474_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139
The candidate 20474_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139 did not pass the final checks
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Considering the candidate 20486_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139
The candidate 20486_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139 did not pass the final checks
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Considering the candidate 20489_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139
The candidate 20489_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139 did not pass the final checks
**** FOUND 01:50:30.97 -23:07:08.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20491_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139
The candidate 20491_fd_For-01-Q1b1x1_2026-08-22_04-38-44_20.00sec_-0.00C_LIGHTs_0139 did not pass the final checks