This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc
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 16.3386 2461268.8386 12.28 04:48:57.38 +27:41:03.6
173.83836 -10.92760 galactic Tau Second-epoch detections are separated by 0.5" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.63 Ausonia 0 1 1 12.5 0 0
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 04:48:57.38 +27:41:03.6: 16.21 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 04:48:57.38 +27:41:03.6: 16.21 +/- 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 16.3386* 04 48 57.38 +27 41 03.6 12.3 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461268.8386,12.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260816.3386 12.28CV 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 16.3386 2461268.8386 12.12 05:10:01.62 +34:35:45.5
171.09228 -3.14126 galactic Aur Second-epoch detections are separated by 1.0" and 4.6 pix
The object was found in VSX 1" NSVS J0510015+343546
Type: L
# Max. Min./Amp. JD0 Period
11.618 R1 Y 0.570 R1 324.000000000000 C
The object was not found in astcheck.
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:10:01.62 +34:35:45.5: 13.09 +/- 0.02 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:10:01.62 +34:35:45.5: 13.10 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0510015+343546,2461268.8386,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0510015+343546 20260816.3386 12.12CV 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 16.3386 2461268.8386 12.88 04:55:22.81 +26:28:38.5
175.70371 -10.55012 galactic Tau Second-epoch detections are separated by 1.0" and 5.3 pix
The object was found in VSX 1" Gaia DR3 153401805018970752
Type: SR|M
# Max. Min./Amp. JD0 Period
12.480 G 12.590 G 351.700000000000 M
The object was not found in astcheck.
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 04:55:22.81 +26:28:38.5: 14.04 +/- 0.06 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 04:55:22.81 +26:28:38.5: 14.00 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.01 +/- 0.04
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 16.3386* 04 55 22.81 +26 28 38.5 12.9 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 153401805018970752,2461268.8386,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 153401805018970752 20260816.3386 12.88CV 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: 2461032.80049318 23.12.2025 07:12:32.611 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
First image: 2461032.80049318 23.12.2025 07:12:32.611 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Last image: 2461268.83892348 16.08.2026 08:07:52.989 /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.59
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 15141
Objects passed selection criteria: 14990
Measurements per detected object (mean, median, min, max): 2.1 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.1 2.0 2 4
Average stars detected per image: 8609.5
Average stars matched: 8324.5 (96.6897 %)
Memory usage VmPeak: 240800 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 Sun Aug 16 03:10:15 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: 2461032.80049318 23.12.2025 07:12:32.611 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
First image: 2461032.80049318 23.12.2025 07:12:32.611 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Last image: 2461268.83892348 16.08.2026 08:07:52.989 /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 29
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.27
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 18 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 116201
Objects passed selection criteria: 115795
Measurements per detected object (mean, median, min, max): 2.2 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.2 2.0 2 4
Average stars detected per image: 68600.2
Average stars matched: 65506.2 (95.4898 %)
Memory usage VmPeak: 578484 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 Sun Aug 16 03:11:15 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits
SExtractor catalog cache: saved Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat to cache
SExtractor catalog cache: saved Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.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/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.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: 2461268.83826873
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_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits exists and is non-empty
wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits exists and is non-empty
wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits exists and is non-empty
wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits (1st reference image)
verification OK: wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Image size: 941.6'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: 05:00:01.042 +29:59:39.82 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_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits (1st new image)
verification OK: wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits
Image size: 944.7'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:00:24.837 +29:57:21.79 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:00:01.042 +29:59:39.82
Second-epoch image center 05:00:24.837 +29:57:21.79
Angular distance between the image centers 0.0941 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits (2nd new image)
verification OK: wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits
Image size: 944.7'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:00:22.555 +29:57:25.40 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:00:01.042 +29:59:39.82
Second-epoch image center 05:00:22.555 +29:57:25.40
Angular distance between the image centers 0.0862 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 05:00:24.837 +29:57:21.79
Second-epoch second image center 05:00:22.555 +29:57:25.40
Angular distance between the image centers 0.00830 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/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits &> /tmp/tmp.iGuhxhaoVv
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits &> /tmp/tmp.YozHa7qoOu
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits &> /tmp/tmp.BKmF1t8ev7
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits &> /tmp/tmp.mthFikCZdh
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.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_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits and wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.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_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits and wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat
Found non-empty wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits and wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat
The reference image (wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits) and catalog (wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat) found
'wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat' -> 'wcsmag.cat'
Read 16295 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 65.5633 to 84.6655 deg, Dec +24.3644 to +35.2863 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 65.5633 to 84.6655 deg, Dec 24.3644 to 35.2863 deg
Loaded 8426 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): 6039 out of 6740 total matches.
Matched with Tycho-2 6740 out of 16295 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.988300
a=0.000000 b=1.000000 c=22.988300
From vast_summary.log: estimated ref. image limiting mag.: -7.59
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.40
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.40
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 16295 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 65.5633 to 84.6655 deg, Dec +24.3644 to +35.2863 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 65.5633 to 84.6655 deg, Dec 24.3644 to 35.2863 deg
Loaded 8426 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): 6039 out of 6740 total matches.
Matched with Tycho-2 6740 out of 16295 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Forced-photometry filter: calibrated wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits -> calib.txt_param_ref_wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits (aperture=6.0)
Read 16349 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 65.5633 to 84.6688 deg, Dec +24.3644 to +35.2864 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 65.5633 to 84.6688 deg, Dec 24.3644 to 35.2864 deg
Loaded 8429 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): 6042 out of 6743 total matches.
Matched with Tycho-2 6743 out of 16349 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
Forced-photometry filter: calibrated wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits -> calib.txt_param_ref_wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits (aperture=6.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
1.9 pix Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
2.9 pix fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits
2.9 pix fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits
Limiting magnitude estimates:
15.4 mag. Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
15.4 mag. Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
12.2 mag. fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits
12.5 mag. fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits
All-image limiting magnitude estimate: 12.2 (SNR ) 10.4 (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.iGuhxhaoVv (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits' -> 'wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.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/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
WCS_IMAGE_NAME=wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
WCS-calibrated image found: wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Checking if the catalog wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat corresponding to the image wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits alredy exist and is non-empty...
Catalog wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat corresponding to the image wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
WCS catalog name: wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1498, bad_region=0, passed=16295
Got 16295 stars (including 14768 good ones) from the SExtractor catalog wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat
util/solve_plate_with_UCAC5 got 16295 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 4837 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4802 matched stars entering correct_measured_positions(), 4802 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4802 matched stars entering correct_measured_positions(), 16295 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 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 4837 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4801 matched stars entering correct_measured_positions(), 16295 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4801 matched stars entering correct_measured_positions(), 16295 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 4801 stars left (next iteration limit 5282)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits N_match=4801 sigma_overall_arcsec=0.373 sigma_q1_arcsec=0.415 sigma_q2_arcsec=0.314 sigma_q3_arcsec=0.346 sigma_q4_arcsec=0.267 n_q1=2038 n_q2=976 n_q3=1109 n_q4=678 worst_quadrant_to_overall_ratio=1.114
The image catalog is written to wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits -region wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.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.YozHa7qoOu (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits' -> 'wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.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/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
WCS_IMAGE_NAME=wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
WCS-calibrated image found: wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
Checking if the catalog wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.wcscat corresponding to the image wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits alredy exist and is non-empty...
Catalog wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.wcscat corresponding to the image wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
WCS catalog name: wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1486, bad_region=0, passed=16349
Got 16349 stars (including 14839 good ones) from the SExtractor catalog wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.wcscat
util/solve_plate_with_UCAC5 got 16349 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 4838 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4801 matched stars entering correct_measured_positions(), 4801 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4801 matched stars entering correct_measured_positions(), 16349 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 571 to 628 (Dec 24.4 to 35.3)
Done reading UCAC5 zone files...
Matched 4838 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4800 matched stars entering correct_measured_positions(), 16349 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4800 matched stars entering correct_measured_positions(), 16349 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 4800 stars left (next iteration limit 5281)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits N_match=4800 sigma_overall_arcsec=0.367 sigma_q1_arcsec=0.414 sigma_q2_arcsec=0.312 sigma_q3_arcsec=0.336 sigma_q4_arcsec=0.273 n_q1=2037 n_q2=978 n_q3=1111 n_q4=674 worst_quadrant_to_overall_ratio=1.129
The image catalog is written to wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits -region wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.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.BKmF1t8ev7 (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_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.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_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits
WCS_IMAGE_NAME=wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits
WCS-calibrated image found: wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits
Checking if the catalog wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits.wcscat corresponding to the image wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits.wcscat corresponding to the image wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits
WCS catalog name: wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=25, bad_region=0, passed=985
Got 985 stars (including 960 good ones) from the SExtractor catalog wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits.wcscat
util/solve_plate_with_UCAC5 got 985 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.7'
Seting catalog search parameters based on the expected field of view 944.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013121 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010497 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 627 (Dec 24.2 to 35.2)
Done reading UCAC5 zone files...
Matched 923 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 912 matched stars entering correct_measured_positions(), 879 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 912 matched stars entering correct_measured_positions(), 942 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 627 (Dec 24.2 to 35.2)
Done reading UCAC5 zone files...
Matched 923 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 914 matched stars entering correct_measured_positions(), 940 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Accuracy estimation diagnostic: 914 matched stars entering correct_measured_positions(), 940 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 914 stars left (next iteration limit 1003)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=914 robust_rms=4.266 arcsec worst_quadrant_rms=9.965 arcsec
SIP_REFIT: SIP order 3 trial: matched=914 robust_rms=0.592 arcsec worst_quadrant_rms=0.798 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=914 robust_rms_before=1.682 arcsec robust_rms_before_corrected=0.601 arcsec robust_rms_after=0.592 arcsec worst_quadrant_rms_before=0.792 worst_quadrant_rms_after=0.798
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.792 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits N_match=914 sigma_overall_arcsec=0.605 sigma_q1_arcsec=0.559 sigma_q2_arcsec=0.757 sigma_q3_arcsec=0.523 sigma_q4_arcsec=0.669 n_q1=309 n_q2=334 n_q3=141 n_q4=130 worst_quadrant_to_overall_ratio=1.252
The image catalog is written to wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits -region wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.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.mthFikCZdh (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_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.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_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits
WCS_IMAGE_NAME=wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits
WCS-calibrated image found: wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits
Checking if the catalog wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits.wcscat corresponding to the image wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits.wcscat corresponding to the image wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits
WCS catalog name: wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=36, bad_region=0, passed=1043
Got 1043 stars (including 1007 good ones) from the SExtractor catalog wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits.wcscat
util/solve_plate_with_UCAC5 got 1043 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.7'
Seting catalog search parameters based on the expected field of view 944.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013121 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010497 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 571 to 627 (Dec 24.2 to 35.2)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 920 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 1007 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
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 571 to 627 (Dec 24.2 to 35.2)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 1008 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 1008 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 954 stars left (next iteration limit 1046)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=954 robust_rms=8.811 arcsec worst_quadrant_rms=11.277 arcsec
SIP_REFIT: SIP order 3 trial: matched=954 robust_rms=0.721 arcsec worst_quadrant_rms=0.984 arcsec
SIP_REFIT: selected SIP order 3
SIP_REFIT: order=3 matched=954 robust_rms_before=1.572 arcsec robust_rms_before_corrected=0.619 arcsec robust_rms_after=0.721 arcsec worst_quadrant_rms_before=0.918 worst_quadrant_rms_after=0.984
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.918 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits N_match=954 sigma_overall_arcsec=0.592 sigma_q1_arcsec=0.452 sigma_q2_arcsec=0.712 sigma_q3_arcsec=0.452 sigma_q4_arcsec=0.785 n_q1=312 n_q2=278 n_q3=140 n_q4=224 worst_quadrant_to_overall_ratio=1.326
The image catalog is written to wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits -region wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.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_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits to local_wcs_cache/
'wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits' -> 'local_wcs_cache/wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits'
Saving the final (post-refit) wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits to local_wcs_cache/
'wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits' -> 'local_wcs_cache/wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits'
Saving the final (post-refit) wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits to local_wcs_cache/
'wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits' -> 'local_wcs_cache/wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits'
Saving the final (post-refit) wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits to local_wcs_cache/
'wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits' -> 'local_wcs_cache/wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits sigma_overall=0.373 worst_q_ratio=1.114
ref2=Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits sigma_overall=0.367 worst_q_ratio=1.129
new1=fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits sigma_overall=0.605 worst_q_ratio=1.252
new2=fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits sigma_overall=0.592 worst_q_ratio=1.326
reference average sigma_overall=0.37 worst_q_ratio=1.1215
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362_astrometric_residuals.png (4801 matched stars from wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.32 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363_astrometric_residuals.png (4800 matched stars from wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.32 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007_astrometric_residuals.png (914 matched stars from wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.56 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008_astrometric_residuals.png (954 matched stars from wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.55 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits'
Saving fully-calibrated image wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits'
Preparing the HTML report for the field Aur-05-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Aur-05-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits
SExtractor catalog cache: saved Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.cat to cache
SExtractor catalog cache: saved Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Creating symlink local_wcs_cache/wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.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_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits exists and is non-empty
wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits exists and is non-empty
wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits exists and is non-empty
wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits (1st reference image)
verification OK: wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Image size: 941.6'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: 05:00:01.042 +29:59:39.82 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_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits (1st new image)
verification OK: wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits
Image size: 944.7'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:00:24.837 +29:57:21.79 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:00:01.042 +29:59:39.82
Second-epoch image center 05:00:24.837 +29:57:21.79
Angular distance between the image centers 0.0941 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits (2nd new image)
verification OK: wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits
Image size: 944.7'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.92"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 05:00:22.555 +29:57:25.40 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:00:01.042 +29:59:39.82
Second-epoch image center 05:00:22.555 +29:57:25.40
Angular distance between the image centers 0.0862 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 05:00:24.837 +29:57:21.79
Second-epoch second image center 05:00:22.555 +29:57:25.40
Angular distance between the image centers 0.00830 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/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits &> /tmp/tmp.7M2VsjWyz5
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits &> /tmp/tmp.CGGw9TPZFP
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits &> /tmp/tmp.VRa0FotZCa
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits &> /tmp/tmp.3pfaYWPOs3
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.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_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits and wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.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_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits and wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat
Found non-empty wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits and wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat
The reference image (wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits) and catalog (wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat) found
'wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat' -> 'wcsmag.cat'
Read 129003 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 65.5559 to 84.6888 deg, Dec +24.3225 to +35.3000 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 65.5559 to 84.6888 deg, Dec 24.3225 to 35.3000 deg
Loaded 8484 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): 4942 out of 6872 total matches.
Matched with Tycho-2 6872 out of 129003 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.844750
a=0.000000 b=1.000000 c=22.844750
From vast_summary.log: estimated ref. image limiting mag.: -7.27
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.57
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.57
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 129003 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 65.5559 to 84.6888 deg, Dec +24.3225 to +35.3000 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 65.5559 to 84.6888 deg, Dec 24.3225 to 35.3000 deg
Loaded 8484 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): 4942 out of 6872 total matches.
Matched with Tycho-2 6872 out of 129003 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Forced-photometry filter: calibrated wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits -> calib.txt_param_ref_wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits (aperture=4.5)
Read 129055 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 65.5633 to 84.6902 deg, Dec +24.3185 to +35.2955 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 65.5633 to 84.6902 deg, Dec 24.3185 to 35.2955 deg
Loaded 8479 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): 4936 out of 6881 total matches.
Matched with Tycho-2 6881 out of 129055 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
Forced-photometry filter: calibrated wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits -> calib.txt_param_ref_wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits (aperture=4.5)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 25 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.8 pix Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
1.9 pix Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
2.6 pix fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits
2.6 pix fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits
Limiting magnitude estimates:
15.6 mag. Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
15.6 mag. Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
13.1 mag. fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits
13.3 mag. fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits
All-image limiting magnitude estimate: 13.1 (SNR ) 12.7 (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.7M2VsjWyz5 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits' -> 'wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.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/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
WCS_IMAGE_NAME=wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
WCS-calibrated image found: wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
Checking if the catalog wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat corresponding to the image wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits alredy exist and is non-empty...
Catalog wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat corresponding to the image wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits
WCS catalog name: wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=36, blended=14027, bad_region=9, passed=128967
Got 128967 stars (including 114713 good ones) from the SExtractor catalog wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat
util/solve_plate_with_UCAC5 got 128967 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 4817 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4789 matched stars entering correct_measured_positions(), 4789 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4789 matched stars entering correct_measured_positions(), 128960 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 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 4817 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4789 matched stars entering correct_measured_positions(), 128960 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4789 matched stars entering correct_measured_positions(), 128960 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 4789 stars left (next iteration limit 5267)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.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_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits N_match=4789 sigma_overall_arcsec=0.358 sigma_q1_arcsec=0.391 sigma_q2_arcsec=0.300 sigma_q3_arcsec=0.339 sigma_q4_arcsec=0.266 n_q1=1871 n_q2=1035 n_q3=1152 n_q4=731 worst_quadrant_to_overall_ratio=1.094
The image catalog is written to wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits -region wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.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.CGGw9TPZFP (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits' -> 'wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.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/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
WCS_IMAGE_NAME=wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
WCS-calibrated image found: wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
Checking if the catalog wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.wcscat corresponding to the image wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits alredy exist and is non-empty...
Catalog wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.wcscat corresponding to the image wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits
WCS catalog name: wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=35, blended=13827, bad_region=12, passed=129020
Got 129020 stars (including 114961 good ones) from the SExtractor catalog wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.wcscat
util/solve_plate_with_UCAC5 got 129020 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 4819 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4791 matched stars entering correct_measured_positions(), 4791 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4791 matched stars entering correct_measured_positions(), 129013 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 571 to 628 (Dec 24.3 to 35.3)
Done reading UCAC5 zone files...
Matched 4819 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4791 matched stars entering correct_measured_positions(), 129013 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4791 matched stars entering correct_measured_positions(), 129013 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 4791 stars left (next iteration limit 5270)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.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_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits N_match=4791 sigma_overall_arcsec=0.363 sigma_q1_arcsec=0.393 sigma_q2_arcsec=0.313 sigma_q3_arcsec=0.348 sigma_q4_arcsec=0.254 n_q1=1874 n_q2=1046 n_q3=1148 n_q4=723 worst_quadrant_to_overall_ratio=1.083
The image catalog is written to wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits -region wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.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.VRa0FotZCa (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_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.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_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits
WCS_IMAGE_NAME=wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits
WCS-calibrated image found: wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits
Checking if the catalog wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits.wcscat corresponding to the image wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits.wcscat corresponding to the image wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits
WCS catalog name: wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=164, bad_region=3, passed=9313
Got 9313 stars (including 9141 good ones) from the SExtractor catalog wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits.wcscat
util/solve_plate_with_UCAC5 got 9313 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.7'
Seting catalog search parameters based on the expected field of view 944.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013121 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010497 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 628 (Dec 24.0 to 35.3)
Done reading UCAC5 zone files...
Matched 4800 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4747 matched stars entering correct_measured_positions(), 4747 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4747 matched stars entering correct_measured_positions(), 9308 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
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 570 to 628 (Dec 24.0 to 35.3)
Done reading UCAC5 zone files...
Matched 4797 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4746 matched stars entering correct_measured_positions(), 9308 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.78"
Accuracy estimation diagnostic: 4746 matched stars entering correct_measured_positions(), 9308 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.79"
Excluding outliers - 4746 stars left (next iteration limit 5221)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.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=4746 robust_rms=4.662 arcsec worst_quadrant_rms=8.618 arcsec
SIP_REFIT: SIP order 3 trial: matched=4746 robust_rms=0.934 arcsec worst_quadrant_rms=1.210 arcsec
SIP_REFIT: SIP order 5 trial: matched=4746 robust_rms=0.806 arcsec worst_quadrant_rms=0.922 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4746 robust_rms_before=1.769 arcsec robust_rms_before_corrected=0.835 arcsec robust_rms_after=0.806 arcsec worst_quadrant_rms_before=0.971 worst_quadrant_rms_after=0.922
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.971 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits N_match=4746 sigma_overall_arcsec=0.801 sigma_q1_arcsec=0.753 sigma_q2_arcsec=0.909 sigma_q3_arcsec=0.680 sigma_q4_arcsec=0.819 n_q1=1475 n_q2=1667 n_q3=831 n_q4=773 worst_quadrant_to_overall_ratio=1.134
The image catalog is written to wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits -region wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.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.3pfaYWPOs3 (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_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.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_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits
WCS_IMAGE_NAME=wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits
WCS-calibrated image found: wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits
Checking if the catalog wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits.wcscat corresponding to the image wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits.wcscat corresponding to the image wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits
WCS catalog name: wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=225, bad_region=6, passed=9020
Got 9020 stars (including 8778 good ones) from the SExtractor catalog wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits.wcscat
util/solve_plate_with_UCAC5 got 9020 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 944.7'
Seting catalog search parameters based on the expected field of view 944.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013121 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010497 (37.8 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 628 (Dec 24.0 to 35.2)
Done reading UCAC5 zone files...
Matched 4797 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4742 matched stars entering correct_measured_positions(), 4735 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.78"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4742 matched stars entering correct_measured_positions(), 9002 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.75"
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 570 to 628 (Dec 24.0 to 35.2)
Done reading UCAC5 zone files...
Matched 4794 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4741 matched stars entering correct_measured_positions(), 9002 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
Accuracy estimation diagnostic: 4741 matched stars entering correct_measured_positions(), 9002 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.78"
Excluding outliers - 4741 stars left (next iteration limit 5216)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.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=4741 robust_rms=6.401 arcsec worst_quadrant_rms=8.925 arcsec
SIP_REFIT: SIP order 3 trial: matched=4741 robust_rms=1.000 arcsec worst_quadrant_rms=1.391 arcsec
SIP_REFIT: SIP order 5 trial: matched=4741 robust_rms=0.811 arcsec worst_quadrant_rms=0.977 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4741 robust_rms_before=1.730 arcsec robust_rms_before_corrected=0.847 arcsec robust_rms_after=0.811 arcsec worst_quadrant_rms_before=0.992 worst_quadrant_rms_after=0.977
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.992 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits N_match=4741 sigma_overall_arcsec=0.811 sigma_q1_arcsec=0.691 sigma_q2_arcsec=0.975 sigma_q3_arcsec=0.640 sigma_q4_arcsec=0.926 n_q1=1513 n_q2=1347 n_q3=739 n_q4=1142 worst_quadrant_to_overall_ratio=1.203
The image catalog is written to wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits -region wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.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_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.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_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-06-56_20.00sec_-0.00C_LIGHTs_0007.fits
Saving fully-calibrated image wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.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_2026-08-16_CI_Aur-05-Q1b1x1_030832_TTUQ1b1x1_943433_Hhit6yuc/wcs_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008.fits
Preparing the HTML report for the field Aur-05-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 04:48:57.38 +27:41:03.6: 16.21 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 04:48:57.38 +27:41:03.6: 16.21 +/- 99.00 upperlimit
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 05:10:01.62 +34:35:45.5: 13.09 +/- 0.02 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 05:10:01.62 +34:35:45.5: 13.10 +/- 0.02 detection
Forced photometry reference-image weighted average: 13.09 +/- 0.02
Forced photometry filter KEPT candidate at 05:10:01.62 +34:35:45.5: ref_mag=13.09 +/- 0.02 new_mean_mag=12.1337 delta=0.96 (need > 0.90)
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-12-32_20.00sec_-15.00C_LIGHT_0362.fits at 04:55:22.81 +26:28:38.5: 14.04 +/- 0.06 detection
Forced photometry on wcs_Aur-05-Q1b1x1_2025-12-23_01-13-14_20.00sec_-14.90C_LIGHT_0363.fits at 04:55:22.81 +26:28:38.5: 14.00 +/- 0.05 detection
Forced photometry reference-image weighted average: 14.01 +/- 0.04
Forced photometry filter KEPT candidate at 04:55:22.81 +26:28:38.5: ref_mag=14.01 +/- 0.04 new_mean_mag=12.8868 delta=1.13 (need > 0.90)
Adding exclusion_list_local.txt__out07926.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out151194.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out98602.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: 3s
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Considering the candidate 151101_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008
The candidate 151101_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008 did not pass the final checks
Rejecting candidate due to large distance (28.5") between the two second-epoch detections
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Considering the candidate 151164_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008
The candidate 151164_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008 did not pass the final checks
Rejecting candidate due to large distance (29.0") between the two second-epoch detections
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Considering the candidate 151194_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008
Preparing report for the candidate 151194_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008
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Considering the candidate 151219_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008
The candidate 151219_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008 did not pass the final checks
**** FOUND 05:19:43.82 +26:10:36.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 151228_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008
The candidate 151228_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008 did not pass the final checks
Rejecting candidate due to large distance (26.3") between the two second-epoch detections
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Considering the candidate 151247_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008
The candidate 151247_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008 did not pass the final checks
**** FOUND 05:05:46.03 +26:25:46.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 151248_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008
The candidate 151248_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008 did not pass the final checks
Rejecting candidate due to large distance (29.2") between the two second-epoch detections
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Considering the candidate 108616_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008
The candidate 108616_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008 did not pass the final checks
**** FOUND 05:06:08.15 +27:03:20.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 116029_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008
The candidate 116029_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008 did not pass the final checks
**** FOUND 04:57:55.34 +27:35:36.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57431_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008
The candidate 57431_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008 did not pass the final checks
**** FOUND 04:54:58.11 +31:19:13.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 104277_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008
The candidate 104277_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008 did not pass the final checks
**** FOUND 05:05:51.03 +26:46:29.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 112628_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008
The candidate 112628_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008 did not pass the final checks
**** FOUND 04:54:57.45 +26:25:39.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105568_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008
The candidate 105568_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008 did not pass the final checks
**** FOUND 05:15:47.47 +26:45:15.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103686_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008
The candidate 103686_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008 did not pass the final checks
**** FOUND 05:02:41.63 +26:45:46.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 96888_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008
The candidate 96888_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008 did not pass the final checks
**** FOUND 05:05:09.02 +25:22:07.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 97196_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008
The candidate 97196_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008 did not pass the final checks
**** FOUND 05:04:49.28 +25:24:55.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103574_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008
The candidate 103574_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008 did not pass the final checks
**** FOUND 04:46:44.48 +26:23:07.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 07926_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008
Preparing report for the candidate 07926_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008
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Considering the candidate 101102_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008
The candidate 101102_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008 did not pass the final checks
**** FOUND 04:51:12.28 +25:58:29.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107910_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008
The candidate 107910_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008 did not pass the final checks
**** FOUND 05:09:07.39 +26:08:20.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 95321_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008
The candidate 95321_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008 did not pass the final checks
**** FOUND 05:18:54.70 +25:01:22.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103136_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008
The candidate 103136_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008 did not pass the final checks
**** FOUND 05:14:36.64 +25:59:35.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103810_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008
The candidate 103810_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008 did not pass the final checks
**** FOUND 05:08:43.30 +26:03:11.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 111199_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008
The candidate 111199_fd_Aur-05-Q1b1x1_2026-08-16_03-07-52_20.00sec_-0.00C_LIGHTs_0008 did not pass the final checks