This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP
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 18.3943 2461270.8943 12.80 02:18:17.54 -00:11:45.0
164.26821 -55.93396 galactic Cet Second-epoch detections are separated by 0.3" and 7.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.505 Cava -0 -0 0 12.8 0 0
Forced photometry on wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits at 02:18:17.54 -00:11:45.0: 16.05 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits at 02:18:17.54 -00:11:45.0: 16.02 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 18.3943* 02 18 17.54 +00 11 45.0 12.8 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
VARIABLE_NAME,2461270.8943,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260818.3943 12.80CV 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 18.3943 2461270.8943 14.85 02:20:28.10 -03:54:08.7
169.28449 -58.51738 galactic Cet Second-epoch detections are separated by 1.0" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.891 Gunhild -0 0 0 14.9 0 0
Forced photometry on wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits at 02:20:28.10 -03:54:08.7: 16.02 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits at 02:20:28.10 -03:54:08.7: 16.04 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 18.3943* 02 20 28.10 -03 54 08.7 14.8 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
VARIABLE_NAME,2461270.8943,14.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260818.3943 14.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.64292808 09.01.2026 03:25:38.986 /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits
First image: 2461049.64292808 09.01.2026 03:25:38.986 /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits
Last image: 2461270.89461529 18.08.2026 09:28:04.761 /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.65
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): 5909
Objects passed selection criteria: 5896
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 4577.25
Average stars matched: 4191.5 (91.5725 %)
Memory usage VmPeak: 231848 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Aug 14 19:27:11 CDT 2026
VaST build number 1.0rc89-191-g1c132b07
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-14)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Aug 18 04:47:07 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.64292808 09.01.2026 03:25:38.986 /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits
First image: 2461049.64292808 09.01.2026 03:25:38.986 /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits
Last image: 2461270.89461529 18.08.2026 09:28:04.761 /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 22
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.34
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 9 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 32111
Objects passed selection criteria: 32018
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 25646.5
Average stars matched: 23453.5 (91.4491 %)
Memory usage VmPeak: 252388 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Aug 14 19:27:11 CDT 2026
VaST build number 1.0rc89-191-g1c132b07
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-14)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Aug 18 04:47:49 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits
SExtractor catalog cache: saved Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits.cat to cache
SExtractor catalog cache: saved Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.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/Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.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: 2461270.89400191
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_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits exists and is non-empty
wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits exists and is non-empty
wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits exists and is non-empty
wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits (1st reference image)
verification OK: wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits
Image size: 941.5'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 02:34:17.849 -02:00:16.62 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_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits (1st new image)
verification OK: wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits
Image size: 937.3'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 02:34:03.300 -01:56:37.85 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 02:34:17.849 -02:00:16.62
Second-epoch image center 02:34:03.300 -01:56:37.85
Angular distance between the image centers 0.0858 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits (2nd new image)
verification OK: wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits
Image size: 937.3'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 02:34:00.756 -01:57:02.48 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 02:34:17.849 -02:00:16.62
Second-epoch image center 02:34:00.756 -01:57:02.48
Angular distance between the image centers 0.0893 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 02:34:03.300 -01:56:37.85
Second-epoch second image center 02:34:00.756 -01:57:02.48
Angular distance between the image centers 0.01261 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/Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits &> /tmp/tmp.MbWfuxpC6X
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits &> /tmp/tmp.HysC9OvKDy
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits &> /tmp/tmp.ccnTxgSksr
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits &> /tmp/tmp.hY07pPTrmL
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits
Calibrating the magnitude scale
Found non-empty wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.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_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits and wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.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_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits and wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits.wcscat
Found non-empty wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits and wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits.wcscat
The reference image (wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits) and catalog (wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits.wcscat) found
'wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits.wcscat' -> 'wcsmag.cat'
Read 6487 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 30.6680 to 46.5230 deg, Dec -7.3087 to +3.3180 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 30.6680 to 46.5230 deg, Dec -7.3087 to 3.3180 deg
Loaded 4175 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): 3371 out of 3568 total matches.
Matched with Tycho-2 3568 out of 6487 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.896100
a=0.000000 b=1.000000 c=22.896100
From vast_summary.log: estimated ref. image limiting mag.: -7.65
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.25
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.25
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 6487 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 30.6680 to 46.5230 deg, Dec -7.3087 to +3.3180 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 30.6680 to 46.5230 deg, Dec -7.3087 to 3.3180 deg
Loaded 4175 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): 3371 out of 3568 total matches.
Matched with Tycho-2 3568 out of 6487 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits
Forced-photometry filter: calibrated wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits -> calib.txt_param_ref_wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits (aperture=5.9)
Read 6467 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 30.6622 to 46.5229 deg, Dec -7.3144 to +3.3098 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 30.6622 to 46.5229 deg, Dec -7.3144 to 3.3098 deg
Loaded 4174 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): 3349 out of 3556 total matches.
Matched with Tycho-2 3556 out of 6467 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits
Forced-photometry filter: calibrated wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits -> calib.txt_param_ref_wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits (aperture=5.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits
2.0 pix Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits
2.3 pix fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits
2.3 pix fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits
Limiting magnitude estimates:
15.2 mag. Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits
15.2 mag. Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits
14.9 mag. fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits
14.9 mag. fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits
All-image limiting magnitude estimate: 14.9 (SNR ) 11.9 (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.MbWfuxpC6X (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits' -> 'wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.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/Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits
WCS_IMAGE_NAME=wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits
WCS-calibrated image found: wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits
Checking if the catalog wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits.wcscat corresponding to the image wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits alredy exist and is non-empty...
Catalog wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits.wcscat corresponding to the image wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits
WCS catalog name: wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=509, bad_region=1489, passed=6487
Got 6487 stars (including 4593 good ones) from the SExtractor catalog wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits.wcscat
util/solve_plate_with_UCAC5 got 6487 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4486 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4480 matched stars entering correct_measured_positions(), 4480 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4480 matched stars entering correct_measured_positions(), 5298 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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4486 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4479 matched stars entering correct_measured_positions(), 5298 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4479 matched stars entering correct_measured_positions(), 5298 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4479 stars left (next iteration limit 4928)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits N_match=4479 sigma_overall_arcsec=0.330 sigma_q1_arcsec=0.438 sigma_q2_arcsec=0.302 sigma_q3_arcsec=0.282 sigma_q4_arcsec=0.271 n_q1=1494 n_q2=799 n_q3=1399 n_q4=787 worst_quadrant_to_overall_ratio=1.330
The image catalog is written to wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits -region wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.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.HysC9OvKDy (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits' -> 'wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.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/Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits
WCS_IMAGE_NAME=wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits
WCS-calibrated image found: wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits
Checking if the catalog wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits.wcscat corresponding to the image wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits alredy exist and is non-empty...
Catalog wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits.wcscat corresponding to the image wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits
WCS catalog name: wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=518, bad_region=1483, passed=6467
Got 6467 stars (including 4560 good ones) from the SExtractor catalog wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits.wcscat
util/solve_plate_with_UCAC5 got 6467 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4455 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4447 matched stars entering correct_measured_positions(), 4447 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4447 matched stars entering correct_measured_positions(), 5280 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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4455 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4446 matched stars entering correct_measured_positions(), 5280 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4446 matched stars entering correct_measured_positions(), 5280 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4446 stars left (next iteration limit 4891)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits N_match=4446 sigma_overall_arcsec=0.333 sigma_q1_arcsec=0.432 sigma_q2_arcsec=0.300 sigma_q3_arcsec=0.294 sigma_q4_arcsec=0.290 n_q1=1469 n_q2=802 n_q3=1381 n_q4=794 worst_quadrant_to_overall_ratio=1.297
The image catalog is written to wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits -region wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.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.ccnTxgSksr (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_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.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_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits
WCS_IMAGE_NAME=wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits
WCS-calibrated image found: wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits
Checking if the catalog wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits.wcscat corresponding to the image wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits alredy exist and is non-empty...
Catalog wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits.wcscat corresponding to the image wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits
WCS catalog name: wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=367, bad_region=1271, passed=5490
Got 5490 stars (including 3925 good ones) from the SExtractor catalog wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits.wcscat
util/solve_plate_with_UCAC5 got 5490 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.2 to 3.3)
Done reading UCAC5 zone files...
Matched 3834 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3826 matched stars entering correct_measured_positions(), 3827 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3826 matched stars entering correct_measured_positions(), 4449 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
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 413 to 468 (Dec -7.2 to 3.3)
Done reading UCAC5 zone files...
Matched 3835 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3827 matched stars entering correct_measured_positions(), 4449 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 3827 matched stars entering correct_measured_positions(), 4449 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 3827 stars left (next iteration limit 4208)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=3827 robust_rms=7.042 arcsec worst_quadrant_rms=9.269 arcsec
SIP_REFIT: SIP order 3 trial: matched=3827 robust_rms=0.437 arcsec worst_quadrant_rms=0.584 arcsec
SIP_REFIT: SIP order 5 trial: matched=3827 robust_rms=0.349 arcsec worst_quadrant_rms=0.383 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3827 robust_rms_before=0.984 arcsec robust_rms_before_corrected=0.343 arcsec robust_rms_after=0.349 arcsec worst_quadrant_rms_before=0.370 worst_quadrant_rms_after=0.383
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.370 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits N_match=3827 sigma_overall_arcsec=0.355 sigma_q1_arcsec=0.323 sigma_q2_arcsec=0.352 sigma_q3_arcsec=0.400 sigma_q4_arcsec=0.348 n_q1=1179 n_q2=709 n_q3=1195 n_q4=744 worst_quadrant_to_overall_ratio=1.127
The image catalog is written to wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits -region wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.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.hY07pPTrmL (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_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.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_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits
WCS_IMAGE_NAME=wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits
WCS-calibrated image found: wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits
Checking if the catalog wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits.wcscat corresponding to the image wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits alredy exist and is non-empty...
Catalog wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits.wcscat corresponding to the image wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits
WCS catalog name: wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=370, bad_region=1255, passed=5496
Got 5496 stars (including 3942 good ones) from the SExtractor catalog wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits.wcscat
util/solve_plate_with_UCAC5 got 5496 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.2 to 3.3)
Done reading UCAC5 zone files...
Matched 3850 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3845 matched stars entering correct_measured_positions(), 3845 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3845 matched stars entering correct_measured_positions(), 4463 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
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 413 to 468 (Dec -7.2 to 3.3)
Done reading UCAC5 zone files...
Matched 3851 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3845 matched stars entering correct_measured_positions(), 4463 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 3845 matched stars entering correct_measured_positions(), 4463 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 3845 stars left (next iteration limit 4229)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=3845 robust_rms=6.945 arcsec worst_quadrant_rms=8.746 arcsec
SIP_REFIT: SIP order 3 trial: matched=3845 robust_rms=0.436 arcsec worst_quadrant_rms=0.584 arcsec
SIP_REFIT: SIP order 5 trial: matched=3845 robust_rms=0.344 arcsec worst_quadrant_rms=0.372 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3845 robust_rms_before=0.980 arcsec robust_rms_before_corrected=0.341 arcsec robust_rms_after=0.344 arcsec worst_quadrant_rms_before=0.369 worst_quadrant_rms_after=0.372
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.369 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits N_match=3845 sigma_overall_arcsec=0.349 sigma_q1_arcsec=0.321 sigma_q2_arcsec=0.331 sigma_q3_arcsec=0.388 sigma_q4_arcsec=0.355 n_q1=1186 n_q2=715 n_q3=1193 n_q4=751 worst_quadrant_to_overall_ratio=1.112
The image catalog is written to wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits -region wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.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_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits to local_wcs_cache/
'wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits' -> 'local_wcs_cache/wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits'
Saving the final (post-refit) wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits to local_wcs_cache/
'wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits' -> 'local_wcs_cache/wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits'
Saving the final (post-refit) wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits to local_wcs_cache/
'wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits' -> 'local_wcs_cache/wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits'
Saving the final (post-refit) wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits to local_wcs_cache/
'wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits' -> 'local_wcs_cache/wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits sigma_overall=0.330 worst_q_ratio=1.330
ref2=Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits sigma_overall=0.333 worst_q_ratio=1.297
new1=fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits sigma_overall=0.355 worst_q_ratio=1.127
new2=fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits sigma_overall=0.349 worst_q_ratio=1.112
reference average sigma_overall=0.3315 worst_q_ratio=1.3135
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097_astrometric_residuals.png (4479 matched stars from wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.29 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098_astrometric_residuals.png (4446 matched stars from wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.29 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450_astrometric_residuals.png (3827 matched stars from wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451_astrometric_residuals.png (3845 matched stars from wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits'
Saving fully-calibrated image wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits'
Preparing the HTML report for the field Cet-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20320_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451
The candidate 20320_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451 did not pass the final checks
**** FOUND 02:19:28.49 -02:57:57.8 in the exclusion list exclusion_list_bbsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Cet-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
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/Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits
SExtractor catalog cache: saved Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits.cat to cache
SExtractor catalog cache: saved Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits
Creating symlink local_wcs_cache/wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits
Creating symlink local_wcs_cache/wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits
Creating symlink local_wcs_cache/wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.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_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits exists and is non-empty
wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits exists and is non-empty
wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits exists and is non-empty
wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits (1st reference image)
verification OK: wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits
Image size: 941.5'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 02:34:17.849 -02:00:16.62 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_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits (1st new image)
verification OK: wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits
Image size: 937.3'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 02:34:03.300 -01:56:37.85 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 02:34:17.849 -02:00:16.62
Second-epoch image center 02:34:03.300 -01:56:37.85
Angular distance between the image centers 0.0858 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits (2nd new image)
verification OK: wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits
Image size: 937.3'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 02:34:00.756 -01:57:02.48 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 02:34:17.849 -02:00:16.62
Second-epoch image center 02:34:00.756 -01:57:02.48
Angular distance between the image centers 0.0893 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 02:34:03.300 -01:56:37.85
Second-epoch second image center 02:34:00.756 -01:57:02.48
Angular distance between the image centers 0.01261 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/Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits &> /tmp/tmp.P7Jm4ENDWa
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits &> /tmp/tmp.c0iFjfrMiI
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits &> /tmp/tmp.uJvAte2aRQ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits &> /tmp/tmp.nGwGxQRqrX
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits
Calibrating the magnitude scale
Found non-empty wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.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_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits and wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.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_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits and wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits.wcscat
Found non-empty wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits and wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits.wcscat
The reference image (wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits) and catalog (wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits.wcscat) found
'wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits.wcscat' -> 'wcsmag.cat'
Read 34731 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 30.6680 to 46.5317 deg, Dec -7.3105 to +3.3218 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 30.6680 to 46.5317 deg, Dec -7.3105 to 3.3218 deg
Loaded 4180 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): 3259 out of 3624 total matches.
Matched with Tycho-2 3624 out of 34731 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.784300
a=0.000000 b=1.000000 c=22.784300
From vast_summary.log: estimated ref. image limiting mag.: -7.34
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.44
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.44
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 34731 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 30.6680 to 46.5317 deg, Dec -7.3105 to +3.3218 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 30.6680 to 46.5317 deg, Dec -7.3105 to 3.3218 deg
Loaded 4180 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): 3259 out of 3624 total matches.
Matched with Tycho-2 3624 out of 34731 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits
Forced-photometry filter: calibrated wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits -> calib.txt_param_ref_wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits (aperture=4.6)
Read 34698 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 30.6560 to 46.5229 deg, Dec -7.3181 to +3.3098 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 30.6560 to 46.5229 deg, Dec -7.3181 to 3.3098 deg
Loaded 4177 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): 3247 out of 3624 total matches.
Matched with Tycho-2 3624 out of 34698 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits
Forced-photometry filter: calibrated wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits -> calib.txt_param_ref_wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits (aperture=4.6)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 16 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits
1.9 pix Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits
2.1 pix fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits
2.1 pix fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits
Limiting magnitude estimates:
15.4 mag. Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits
15.4 mag. Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits
15.0 mag. fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits
15.0 mag. fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 14.5 (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.P7Jm4ENDWa (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits' -> 'wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.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/Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits
WCS_IMAGE_NAME=wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits
WCS-calibrated image found: wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits
Checking if the catalog wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits.wcscat corresponding to the image wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits alredy exist and is non-empty...
Catalog wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits.wcscat corresponding to the image wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits
WCS catalog name: wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=1492, bad_region=6460, passed=34716
Got 34716 stars (including 26988 good ones) from the SExtractor catalog wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits.wcscat
util/solve_plate_with_UCAC5 got 34716 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4896 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: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4892 matched stars entering correct_measured_positions(), 29638 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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4896 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4891 matched stars entering correct_measured_positions(), 29638 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4891 matched stars entering correct_measured_positions(), 29638 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4891 stars left (next iteration limit 5381)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.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_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits N_match=4891 sigma_overall_arcsec=0.330 sigma_q1_arcsec=0.425 sigma_q2_arcsec=0.310 sigma_q3_arcsec=0.285 sigma_q4_arcsec=0.270 n_q1=1660 n_q2=880 n_q3=1514 n_q4=837 worst_quadrant_to_overall_ratio=1.288
The image catalog is written to wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits -region wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.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.c0iFjfrMiI (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits' -> 'wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.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/Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits
WCS_IMAGE_NAME=wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits
WCS-calibrated image found: wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits
Checking if the catalog wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits.wcscat corresponding to the image wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits alredy exist and is non-empty...
Catalog wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits.wcscat corresponding to the image wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits
WCS catalog name: wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=1502, bad_region=6453, passed=34691
Got 34691 stars (including 26977 good ones) from the SExtractor catalog wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits.wcscat
util/solve_plate_with_UCAC5 got 34691 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 413 to 468 (Dec -7.3 to 3.3)
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: 4889 matched stars entering correct_measured_positions(), 4889 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4889 matched stars entering correct_measured_positions(), 29621 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 413 to 468 (Dec -7.3 to 3.3)
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: 4889 matched stars entering correct_measured_positions(), 29621 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4889 matched stars entering correct_measured_positions(), 29621 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4889 stars left (next iteration limit 5377)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.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_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits N_match=4889 sigma_overall_arcsec=0.335 sigma_q1_arcsec=0.428 sigma_q2_arcsec=0.303 sigma_q3_arcsec=0.288 sigma_q4_arcsec=0.289 n_q1=1653 n_q2=881 n_q3=1509 n_q4=846 worst_quadrant_to_overall_ratio=1.280
The image catalog is written to wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits -region wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.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.uJvAte2aRQ (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_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.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_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits
WCS_IMAGE_NAME=wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits
WCS-calibrated image found: wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits
Checking if the catalog wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits.wcscat corresponding to the image wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits alredy exist and is non-empty...
Catalog wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits.wcscat corresponding to the image wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits
WCS catalog name: wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=1159, bad_region=5278, passed=28627
Got 28627 stars (including 22443 good ones) from the SExtractor catalog wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits.wcscat
util/solve_plate_with_UCAC5 got 28627 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.2 to 3.3)
Done reading UCAC5 zone files...
Matched 4884 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4880 matched stars entering correct_measured_positions(), 4880 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4880 matched stars entering correct_measured_positions(), 24642 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 413 to 468 (Dec -7.2 to 3.3)
Done reading UCAC5 zone files...
Matched 4884 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4880 matched stars entering correct_measured_positions(), 24642 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4880 matched stars entering correct_measured_positions(), 24642 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 4880 stars left (next iteration limit 5368)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.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=4880 robust_rms=6.854 arcsec worst_quadrant_rms=8.810 arcsec
SIP_REFIT: SIP order 3 trial: matched=4880 robust_rms=0.452 arcsec worst_quadrant_rms=0.604 arcsec
SIP_REFIT: SIP order 5 trial: matched=4880 robust_rms=0.358 arcsec worst_quadrant_rms=0.404 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4880 robust_rms_before=0.974 arcsec robust_rms_before_corrected=0.347 arcsec robust_rms_after=0.358 arcsec worst_quadrant_rms_before=0.381 worst_quadrant_rms_after=0.404
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.381 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits N_match=4880 sigma_overall_arcsec=0.359 sigma_q1_arcsec=0.322 sigma_q2_arcsec=0.361 sigma_q3_arcsec=0.408 sigma_q4_arcsec=0.348 n_q1=1537 n_q2=868 n_q3=1534 n_q4=941 worst_quadrant_to_overall_ratio=1.137
The image catalog is written to wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits -region wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.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.nGwGxQRqrX (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_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.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_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits
WCS_IMAGE_NAME=wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits
WCS-calibrated image found: wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits
Checking if the catalog wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits.wcscat corresponding to the image wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits alredy exist and is non-empty...
Catalog wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits.wcscat corresponding to the image wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits
WCS catalog name: wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=1154, bad_region=5251, passed=28654
Got 28654 stars (including 22495 good ones) from the SExtractor catalog wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits.wcscat
util/solve_plate_with_UCAC5 got 28654 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.2 to 3.3)
Done reading UCAC5 zone files...
Matched 4884 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4879 matched stars entering correct_measured_positions(), 4879 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4879 matched stars entering correct_measured_positions(), 24696 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
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 413 to 468 (Dec -7.2 to 3.3)
Done reading UCAC5 zone files...
Matched 4884 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4879 matched stars entering correct_measured_positions(), 24696 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4879 matched stars entering correct_measured_positions(), 24696 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4879 stars left (next iteration limit 5366)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.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=4879 robust_rms=6.836 arcsec worst_quadrant_rms=8.675 arcsec
SIP_REFIT: SIP order 3 trial: matched=4879 robust_rms=0.443 arcsec worst_quadrant_rms=0.587 arcsec
SIP_REFIT: SIP order 5 trial: matched=4879 robust_rms=0.350 arcsec worst_quadrant_rms=0.391 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4879 robust_rms_before=0.969 arcsec robust_rms_before_corrected=0.346 arcsec robust_rms_after=0.350 arcsec worst_quadrant_rms_before=0.380 worst_quadrant_rms_after=0.391
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.380 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits N_match=4879 sigma_overall_arcsec=0.352 sigma_q1_arcsec=0.322 sigma_q2_arcsec=0.332 sigma_q3_arcsec=0.396 sigma_q4_arcsec=0.346 n_q1=1539 n_q2=860 n_q3=1535 n_q4=945 worst_quadrant_to_overall_ratio=1.126
The image catalog is written to wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits -region wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.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_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.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_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-27-11_20.00sec_0.00C_LIGHT_0450.fits
Saving fully-calibrated image wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.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_2026-08-18_CI_Cet-04-Q2b1x1_044249_TTUQ2b1x1_1417775_NEZupfTP/wcs_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451.fits
Preparing the HTML report for the field Cet-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits at 02:51:25.52 +02:09:34.5: 13.92 +/- 0.07 detection
Forced photometry on wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits at 02:45:47.30 -04:57:15.0: 14.01 +/- 0.06 detection
Forced photometry on wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits at 02:17:06.47 -00:30:07.3: 14.31 +/- 0.07 detection
Forced photometry on wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits at 02:29:31.24 -04:58:17.5: 14.40 +/- 0.08 detection
Forced photometry on wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits at 02:18:17.54 -00:11:45.0: 16.05 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits at 02:50:05.43 -04:42:39.5: 13.55 +/- 0.04 detection
Forced photometry on wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits at 02:41:07.81 -04:11:46.1: 14.36 +/- 0.07 detection
Forced photometry on wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits at 02:46:48.02 -04:33:38.8: 14.22 +/- 0.07 detection
Forced photometry on wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits at 02:49:10.39 -02:35:30.8: 14.10 +/- 0.06 detection
Forced photometry on wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits at 02:20:14.02 -03:20:17.4: 15.22 +/- 0.17 detection
Forced photometry on wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits at 02:18:17.54 -00:11:45.0: 16.02 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits at 02:17:06.47 -00:30:07.3: 14.19 +/- 0.07 detection
Forced photometry on wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits at 02:29:31.24 -04:58:17.5: 14.32 +/- 0.08 detection
Forced photometry on wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits at 02:50:05.43 -04:42:39.5: 13.61 +/- 0.05 detection
Forced photometry on wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits at 02:41:07.81 -04:11:46.1: 14.23 +/- 0.07 detection
Forced photometry on wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits at 02:45:47.30 -04:57:15.0: 13.92 +/- 0.05 detection
Forced photometry on wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits at 02:51:25.52 +02:09:34.5: 13.88 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.24 +/- 0.05
Forced photometry reference-image weighted average: 14.36 +/- 0.06
Forced photometry filter REJECTED candidate at 02:17:06.47 -00:30:07.3: ref_mag=14.24 +/- 0.05 new_mean_mag=13.9807 delta=0.26 (need > 0.90)
Forced photometry reference-image weighted average: 14.29 +/- 0.05
Forced photometry filter REJECTED candidate at 02:29:31.24 -04:58:17.5: ref_mag=14.36 +/- 0.06 new_mean_mag=14.3430 delta=0.01 (need > 0.90)
Forced photometry reference-image weighted average: 13.58 +/- 0.03
Forced photometry reference-image weighted average: 13.96 +/- 0.04
Forced photometry reference-image weighted average: 13.90 +/- 0.05
Forced photometry filter REJECTED candidate at 02:41:07.81 -04:11:46.1: ref_mag=14.29 +/- 0.05 new_mean_mag=14.6135 delta=-0.32 (need > 0.90)
Forced photometry filter REJECTED candidate at 02:50:05.43 -04:42:39.5: ref_mag=13.58 +/- 0.03 new_mean_mag=13.7007 delta=-0.12 (need > 0.90)
Forced photometry filter REJECTED candidate at 02:45:47.30 -04:57:15.0: ref_mag=13.96 +/- 0.04 new_mean_mag=14.2082 delta=-0.25 (need > 0.90)
Forced photometry filter REJECTED candidate at 02:51:25.52 +02:09:34.5: ref_mag=13.90 +/- 0.05 new_mean_mag=14.0629 delta=-0.16 (need > 0.90)
Forced photometry on wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits at 02:46:48.02 -04:33:38.8: 14.27 +/- 0.08 detection
Forced photometry on wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits at 02:49:10.39 -02:35:30.8: 14.18 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.24 +/- 0.05
Forced photometry filter REJECTED candidate at 02:46:48.02 -04:33:38.8: ref_mag=14.24 +/- 0.05 new_mean_mag=14.2781 delta=-0.04 (need > 0.90)
Forced photometry reference-image weighted average: 14.14 +/- 0.05
Forced photometry filter REJECTED candidate at 02:49:10.39 -02:35:30.8: ref_mag=14.14 +/- 0.05 new_mean_mag=14.1555 delta=-0.02 (need > 0.90)
Forced photometry on wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits at 02:20:14.02 -03:20:17.4: 15.05 +/- 0.14 detection
Forced photometry reference-image weighted average: 15.12 +/- 0.11
Forced photometry filter REJECTED candidate at 02:20:14.02 -03:20:17.4: ref_mag=15.12 +/- 0.11 new_mean_mag=14.6564 delta=0.46 (need > 0.90)
Forced photometry on wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits at 02:21:36.84 -06:09:27.7: 15.13 +/- 0.17 detection
Forced photometry on wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits at 02:20:28.10 -03:54:08.7: 16.02 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-04-Q2b1x1_2026-01-08_21-25-38_20.00sec_-15.00C_LIGHT_0097.fits at 02:30:10.77 -00:38:55.4: 15.47 +/- 0.19 detection
Forced photometry on wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits at 02:20:28.10 -03:54:08.7: 16.04 +/- 99.00 upperlimit
Forced photometry on wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits at 02:21:36.84 -06:09:27.7: 15.18 +/- 0.17 detection
Forced photometry on wcs_Cet-04-Q2b1x1_2026-01-08_21-26-36_20.00sec_-15.00C_LIGHT_0098.fits at 02:30:10.77 -00:38:55.4: 15.10 +/- 0.14 detection
Forced photometry reference-image weighted average: 15.15 +/- 0.12
Forced photometry reference-image weighted average: 15.23 +/- 0.11
Forced photometry filter REJECTED candidate at 02:21:36.84 -06:09:27.7: ref_mag=15.15 +/- 0.12 new_mean_mag=14.9754 delta=0.18 (need > 0.90)
Forced photometry filter REJECTED candidate at 02:30:10.77 -00:38:55.4: ref_mag=15.23 +/- 0.11 new_mean_mag=14.7504 delta=0.48 (need > 0.90)
Adding exclusion_list_local.txt__out53568.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out57679.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 8s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 51933_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451
The candidate 51933_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451 did not pass the final checks
Rejecting candidate due to large distance (16.0") between the two second-epoch detections
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Considering the candidate 51935_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451
The candidate 51935_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451 did not pass the final checks
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Considering the candidate 51936_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451
The candidate 51936_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451 did not pass the final checks
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Considering the candidate 51940_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451
The candidate 51940_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451 did not pass the final checks
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Considering the candidate 52022_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451
The candidate 52022_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451 did not pass the final checks
**** FOUND 02:19:28.49 -02:57:57.8 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 53568_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451
Preparing report for the candidate 53568_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451
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Considering the candidate 54629_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451
The candidate 54629_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451 did not pass the final checks
**** FOUND 02:19:14.41 -02:56:30.0 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 55183_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451
The candidate 55183_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451 did not pass the final checks
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Considering the candidate 55498_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451
The candidate 55498_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451 did not pass the final checks
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Considering the candidate 55841_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451
The candidate 55841_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451 did not pass the final checks
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Considering the candidate 56363_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451
The candidate 56363_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451 did not pass the final checks
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Considering the candidate 56702_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451
The candidate 56702_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451 did not pass the final checks
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Considering the candidate 57010_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451
The candidate 57010_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451 did not pass the final checks
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Considering the candidate 57452_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451
The candidate 57452_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451 did not pass the final checks
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Considering the candidate 57679_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451
Preparing report for the candidate 57679_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451
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Considering the candidate 57680_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451
The candidate 57680_fd_Cet-04-Q2b1x1_2026-08-18_04-28-04_20.00sec_-0.00C_LIGHT_0451 did not pass the final checks