This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 25.2665* 03 31 11.98 +43 54 14.9 10.9 U Per 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
GK Per,2461277.7665,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GK Per 20260825.2665 10.88CV 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
Mean magnitude and position on the discovery images:
2026 08 25.2665 2461277.7665 13.66 03:02:41.30 +41:33:40.5
147.74012 -14.90226 galactic Per Second-epoch detections are separated by 8.2" and 0.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:02:41.30 +41:33:40.5 (user input) | T | P | (position from user input)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:02:41.30 +41:33:40.5: 15.99 +/- 99.00 upperlimit
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:02:41.30 +41:33:40.5: 15.99 +/- 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 25.2665* 03 02 41.30 +41 33 40.5 13.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461277.7665,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260825.2665 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 08 25.2665* 03 31 11.98 +43 54 14.9 10.9 U Per 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
GK Per,2461277.7665,10.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GK Per 20260825.2665 10.88CV 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: 2461049.58214624 09.01.2026 01:58:07.435 /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
First image: 2461049.58214624 09.01.2026 01:58:07.435 /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
Last image: 2461277.76676347 25.08.2026 06:23:58.364 /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.52
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: 6 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): 18056
Objects passed selection criteria: 17969
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 12281
Average stars matched: 11908.2 (96.9648 %)
Memory usage VmPeak: 244832 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Mon Aug 24 15:05:05 CDT 2026
VaST build number 1.0rc89-195-gae6eb4b1
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-24)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Aug 25 01:27:07 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.58214624 09.01.2026 01:58:07.435 /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
First image: 2461049.58214624 09.01.2026 01:58:07.435 /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
Last image: 2461277.76676347 25.08.2026 06:23:58.364 /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 83
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.19
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: 38 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): 141536
Objects passed selection criteria: 141138
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 101580
Average stars matched: 98029.2 (96.505 %)
Memory usage VmPeak: 561284 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Mon Aug 24 15:05:05 CDT 2026
VaST build number 1.0rc89-195-gae6eb4b1
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-08-24)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Tue Aug 25 01:28:45 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits
SExtractor catalog cache: saved Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.cat to cache
SExtractor catalog cache: saved Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.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/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.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: 2461277.76630360
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_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits exists and is non-empty
wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits exists and is non-empty
wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits exists and is non-empty
wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits (1st reference image)
verification OK: wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
Image size: 941.5'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 03:36:01.913 +46:00:00.61 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_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits (1st new image)
verification OK: wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits
Image size: 938.1'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 03:36:01.658 +45:59:38.43 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 03:36:01.913 +46:00:00.61
Second-epoch image center 03:36:01.658 +45:59:38.43
Angular distance between the image centers 0.0062 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits (2nd new image)
verification OK: wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits
Image size: 938.1'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 03:36:00.736 +45:59:37.72 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 03:36:01.913 +46:00:00.61
Second-epoch image center 03:36:00.736 +45:59:37.72
Angular distance between the image centers 0.0072 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 03:36:01.658 +45:59:38.43
Second-epoch second image center 03:36:00.736 +45:59:37.72
Angular distance between the image centers 0.00268 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/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits &> /tmp/tmp.T5fC99dfzV
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits &> /tmp/tmp.FNNyLJ0Xzl
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits &> /tmp/tmp.IyoRoStdZA
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits &> /tmp/tmp.CPIIg1JuDm
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits
Calibrating the magnitude scale
Found non-empty wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.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_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits and wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.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_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits and wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat
Found non-empty wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits and wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat
The reference image (wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits) and catalog (wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat) found
'wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat' -> 'wcsmag.cat'
Read 24919 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 41.2386 to 65.8886 deg, Dec +39.8263 to +51.4097 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 41.2386 to 65.8886 deg, Dec 39.8263 to 51.4097 deg
Loaded 12587 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): 8299 out of 9376 total matches.
Matched with Tycho-2 9376 out of 24919 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.954600
a=0.000000 b=1.000000 c=22.954600
From vast_summary.log: estimated ref. image limiting mag.: -7.52
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.43
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.43
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 24919 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 41.2386 to 65.8886 deg, Dec +39.8263 to +51.4097 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 41.2386 to 65.8886 deg, Dec 39.8263 to 51.4097 deg
Loaded 12587 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): 8299 out of 9376 total matches.
Matched with Tycho-2 9376 out of 24919 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
Forced-photometry filter: calibrated wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits -> calib.txt_param_ref_wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits (aperture=5.7)
Read 25014 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 41.2390 to 65.8888 deg, Dec +39.8264 to +51.4150 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 41.2390 to 65.8888 deg, Dec 39.8264 to 51.4150 deg
Loaded 12591 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): 8306 out of 9365 total matches.
Matched with Tycho-2 9365 out of 25014 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
Forced-photometry filter: calibrated wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits -> calib.txt_param_ref_wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits (aperture=5.8)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
2.0 pix Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
2.3 pix fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits
2.3 pix fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits
Limiting magnitude estimates:
15.4 mag. Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
15.4 mag. Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
13.5 mag. fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits
13.6 mag. fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits
All-image limiting magnitude estimate: 13.5 (SNR ) 10.9 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.T5fC99dfzV (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits' -> 'wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.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/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
WCS_IMAGE_NAME=wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
WCS-calibrated image found: wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
Checking if the catalog wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat corresponding to the image wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits alredy exist and is non-empty...
Catalog wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat corresponding to the image wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
WCS catalog name: wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2608, bad_region=5544, passed=24919
Got 24919 stars (including 17235 good ones) from the SExtractor catalog wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat
util/solve_plate_with_UCAC5 got 24919 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 4940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4918 matched stars entering correct_measured_positions(), 4918 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4918 matched stars entering correct_measured_positions(), 20428 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
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 649 to 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 4940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4919 matched stars entering correct_measured_positions(), 20428 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 4919 matched stars entering correct_measured_positions(), 20428 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 4919 stars left (next iteration limit 5409)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits N_match=4919 sigma_overall_arcsec=0.425 sigma_q1_arcsec=0.552 sigma_q2_arcsec=0.379 sigma_q3_arcsec=0.375 sigma_q4_arcsec=0.379 n_q1=1615 n_q2=801 n_q3=1627 n_q4=876 worst_quadrant_to_overall_ratio=1.300
The image catalog is written to wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits -region wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.FNNyLJ0Xzl (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits' -> 'wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.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/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
WCS_IMAGE_NAME=wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
WCS-calibrated image found: wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
Checking if the catalog wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits.wcscat corresponding to the image wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits alredy exist and is non-empty...
Catalog wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits.wcscat corresponding to the image wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
WCS catalog name: wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=17, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2561, bad_region=5578, passed=24997
Got 24997 stars (including 17348 good ones) from the SExtractor catalog wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits.wcscat
util/solve_plate_with_UCAC5 got 24997 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 4942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4919 matched stars entering correct_measured_positions(), 4919 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4919 matched stars entering correct_measured_positions(), 20490 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 649 to 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 4942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4920 matched stars entering correct_measured_positions(), 20490 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4920 matched stars entering correct_measured_positions(), 20490 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 4920 stars left (next iteration limit 5410)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits N_match=4920 sigma_overall_arcsec=0.382 sigma_q1_arcsec=0.466 sigma_q2_arcsec=0.360 sigma_q3_arcsec=0.350 sigma_q4_arcsec=0.356 n_q1=1613 n_q2=791 n_q3=1642 n_q4=874 worst_quadrant_to_overall_ratio=1.221
The image catalog is written to wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits -region wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.IyoRoStdZA (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_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.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_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits
WCS_IMAGE_NAME=wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits
WCS-calibrated image found: wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits
Checking if the catalog wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits.wcscat corresponding to the image wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits.wcscat corresponding to the image wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits
WCS catalog name: wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=423, bad_region=1033, passed=6305
Got 6305 stars (including 4889 good ones) from the SExtractor catalog wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits.wcscat
util/solve_plate_with_UCAC5 got 6305 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.1'
Seting catalog search parameters based on the expected field of view 938.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013029 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010423 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.2 to 51.2)
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: 4796 matched stars entering correct_measured_positions(), 4796 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4796 matched stars entering correct_measured_positions(), 5480 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.2 to 51.2)
Done reading UCAC5 zone files...
Matched 4821 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4796 matched stars entering correct_measured_positions(), 5480 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Accuracy estimation diagnostic: 4796 matched stars entering correct_measured_positions(), 5480 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 4796 stars left (next iteration limit 5275)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4796 robust_rms=5.638 arcsec worst_quadrant_rms=16.697 arcsec
SIP_REFIT: SIP order 3 trial: matched=4796 robust_rms=0.673 arcsec worst_quadrant_rms=0.764 arcsec
SIP_REFIT: SIP order 5 trial: matched=4796 robust_rms=0.496 arcsec worst_quadrant_rms=0.543 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4796 robust_rms_before=0.982 arcsec robust_rms_before_corrected=0.499 arcsec robust_rms_after=0.496 arcsec worst_quadrant_rms_before=0.544 worst_quadrant_rms_after=0.543
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.544 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits N_match=4796 sigma_overall_arcsec=0.509 sigma_q1_arcsec=0.484 sigma_q2_arcsec=0.531 sigma_q3_arcsec=0.551 sigma_q4_arcsec=0.483 n_q1=1662 n_q2=636 n_q3=1750 n_q4=748 worst_quadrant_to_overall_ratio=1.083
The image catalog is written to wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits -region wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.CPIIg1JuDm (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_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.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_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits
WCS_IMAGE_NAME=wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits
WCS-calibrated image found: wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits
Checking if the catalog wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits.wcscat corresponding to the image wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits.wcscat corresponding to the image wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits
WCS catalog name: wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=441, bad_region=1056, passed=6350
Got 6350 stars (including 4894 good ones) from the SExtractor catalog wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits.wcscat
util/solve_plate_with_UCAC5 got 6350 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.1'
Seting catalog search parameters based on the expected field of view 938.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013029 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010423 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.2 to 51.2)
Done reading UCAC5 zone files...
Matched 4824 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4798 matched stars entering correct_measured_positions(), 4798 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4798 matched stars entering correct_measured_positions(), 5516 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
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 650 to 708 (Dec 40.2 to 51.2)
Done reading UCAC5 zone files...
Matched 4826 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4799 matched stars entering correct_measured_positions(), 5516 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Accuracy estimation diagnostic: 4799 matched stars entering correct_measured_positions(), 5516 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 4799 stars left (next iteration limit 5277)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4799 robust_rms=5.665 arcsec worst_quadrant_rms=16.064 arcsec
SIP_REFIT: SIP order 3 trial: matched=4799 robust_rms=0.650 arcsec worst_quadrant_rms=0.754 arcsec
SIP_REFIT: SIP order 5 trial: matched=4799 robust_rms=0.501 arcsec worst_quadrant_rms=0.569 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4799 robust_rms_before=0.950 arcsec robust_rms_before_corrected=0.507 arcsec robust_rms_after=0.501 arcsec worst_quadrant_rms_before=0.557 worst_quadrant_rms_after=0.569
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.557 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits N_match=4799 sigma_overall_arcsec=0.532 sigma_q1_arcsec=0.493 sigma_q2_arcsec=0.552 sigma_q3_arcsec=0.595 sigma_q4_arcsec=0.453 n_q1=1654 n_q2=666 n_q3=1734 n_q4=745 worst_quadrant_to_overall_ratio=1.118
The image catalog is written to wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits -region wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits to local_wcs_cache/
'wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits' -> 'local_wcs_cache/wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits'
Saving the final (post-refit) wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits to local_wcs_cache/
'wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits' -> 'local_wcs_cache/wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits'
Saving the final (post-refit) wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits to local_wcs_cache/
'wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits' -> 'local_wcs_cache/wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits'
Saving the final (post-refit) wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits to local_wcs_cache/
'wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits' -> 'local_wcs_cache/wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits sigma_overall=0.425 worst_q_ratio=1.300
ref2=Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits sigma_overall=0.382 worst_q_ratio=1.221
new1=fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits sigma_overall=0.509 worst_q_ratio=1.083
new2=fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits sigma_overall=0.532 worst_q_ratio=1.118
reference average sigma_overall=0.4035 worst_q_ratio=1.2605
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020_astrometric_residuals.png (4919 matched stars from wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.39 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021_astrometric_residuals.png (4920 matched stars from wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131_astrometric_residuals.png (4796 matched stars from wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.46 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132_astrometric_residuals.png (4799 matched stars from wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.47 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits'
Saving fully-calibrated image wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits'
Preparing the HTML report for the field Per-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 4s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31458_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
Preparing report for the candidate 31458_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08393_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 08393_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:29:23.35 +44:24:26.6 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 6s
Prepared the HTML report for the field Per-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits
SExtractor catalog cache: saved Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.cat to cache
SExtractor catalog cache: saved Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
Creating symlink local_wcs_cache/wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
Creating symlink local_wcs_cache/wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits
Creating symlink local_wcs_cache/wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.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_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits exists and is non-empty
wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits exists and is non-empty
wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits exists and is non-empty
wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits (1st reference image)
verification OK: wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
Image size: 941.5'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 03:36:01.913 +46:00:00.61 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_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits (1st new image)
verification OK: wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits
Image size: 938.1'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 03:36:01.658 +45:59:38.43 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 03:36:01.913 +46:00:00.61
Second-epoch image center 03:36:01.658 +45:59:38.43
Angular distance between the image centers 0.0062 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits (2nd new image)
verification OK: wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits
Image size: 938.1'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.88"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 03:36:00.736 +45:59:37.72 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 03:36:01.913 +46:00:00.61
Second-epoch image center 03:36:00.736 +45:59:37.72
Angular distance between the image centers 0.0072 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 03:36:01.658 +45:59:38.43
Second-epoch second image center 03:36:00.736 +45:59:37.72
Angular distance between the image centers 0.00268 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/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits &> /tmp/tmp.rd4GlQ8mMb
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits &> /tmp/tmp.WL8dgQJBum
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits &> /tmp/tmp.vFZmMNHgqE
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits &> /tmp/tmp.MqJNrySJZh
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits
Calibrating the magnitude scale
Found non-empty wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.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_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits and wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.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_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits and wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat
Found non-empty wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits and wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat
The reference image (wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits) and catalog (wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat) found
'wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat' -> 'wcsmag.cat'
Read 189134 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 41.2226 to 65.9097 deg, Dec +39.7810 to +51.4146 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 41.2226 to 65.9097 deg, Dec 39.7810 to 51.4146 deg
Loaded 12673 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): 6489 out of 9455 total matches.
Matched with Tycho-2 9455 out of 189134 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.821000
a=0.000000 b=1.000000 c=22.821000
From vast_summary.log: estimated ref. image limiting mag.: -7.19
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.63
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.63
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 189134 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 41.2226 to 65.9097 deg, Dec +39.7810 to +51.4146 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 41.2226 to 65.9097 deg, Dec 39.7810 to 51.4146 deg
Loaded 12673 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): 6489 out of 9455 total matches.
Matched with Tycho-2 9455 out of 189134 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
Forced-photometry filter: calibrated wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits -> calib.txt_param_ref_wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits (aperture=4.3)
Read 187812 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 41.2223 to 65.9102 deg, Dec +39.7810 to +51.4199 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 41.2223 to 65.9102 deg, Dec 39.7810 to 51.4199 deg
Loaded 12677 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): 6500 out of 9428 total matches.
Matched with Tycho-2 9428 out of 187812 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
Forced-photometry filter: calibrated wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits -> calib.txt_param_ref_wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits (aperture=4.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 66 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.8 pix Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
1.9 pix Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
2.2 pix fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits
2.1 pix fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits
Limiting magnitude estimates:
15.6 mag. Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
15.6 mag. Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
13.8 mag. fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits
13.8 mag. fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 13.4 (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.rd4GlQ8mMb (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits' -> 'wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.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/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
WCS_IMAGE_NAME=wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
WCS-calibrated image found: wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
Checking if the catalog wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat corresponding to the image wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits alredy exist and is non-empty...
Catalog wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat corresponding to the image wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits
WCS catalog name: wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=43, blended=23506, bad_region=33336, passed=189091
Got 189091 stars (including 135790 good ones) from the SExtractor catalog wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat
util/solve_plate_with_UCAC5 got 189091 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 648 to 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 4933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4923 matched stars entering correct_measured_positions(), 4923 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4923 matched stars entering correct_measured_positions(), 162706 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
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 648 to 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 4933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4923 matched stars entering correct_measured_positions(), 162706 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 4923 matched stars entering correct_measured_positions(), 162706 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 4923 stars left (next iteration limit 5415)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.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_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits N_match=4923 sigma_overall_arcsec=0.405 sigma_q1_arcsec=0.527 sigma_q2_arcsec=0.369 sigma_q3_arcsec=0.359 sigma_q4_arcsec=0.356 n_q1=1620 n_q2=815 n_q3=1614 n_q4=874 worst_quadrant_to_overall_ratio=1.300
The image catalog is written to wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits -region wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.WL8dgQJBum (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits' -> 'wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.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/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
WCS_IMAGE_NAME=wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
WCS-calibrated image found: wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
Checking if the catalog wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits.wcscat corresponding to the image wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits alredy exist and is non-empty...
Catalog wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits.wcscat corresponding to the image wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits
WCS catalog name: wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=6, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=36, blended=23390, bad_region=33357, passed=187770
Got 187770 stars (including 134514 good ones) from the SExtractor catalog wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits.wcscat
util/solve_plate_with_UCAC5 got 187770 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 648 to 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 4932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4919 matched stars entering correct_measured_positions(), 4919 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4919 matched stars entering correct_measured_positions(), 161324 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 648 to 709 (Dec 39.8 to 51.4)
Done reading UCAC5 zone files...
Matched 4932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4919 matched stars entering correct_measured_positions(), 161324 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 4919 matched stars entering correct_measured_positions(), 161324 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 4919 stars left (next iteration limit 5410)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.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_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits N_match=4919 sigma_overall_arcsec=0.370 sigma_q1_arcsec=0.437 sigma_q2_arcsec=0.354 sigma_q3_arcsec=0.343 sigma_q4_arcsec=0.344 n_q1=1627 n_q2=807 n_q3=1602 n_q4=883 worst_quadrant_to_overall_ratio=1.180
The image catalog is written to wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits -region wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.vFZmMNHgqE (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_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.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_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits
WCS_IMAGE_NAME=wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits
WCS-calibrated image found: wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits
Checking if the catalog wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits.wcscat corresponding to the image wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits.wcscat corresponding to the image wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits
WCS catalog name: wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=2585, bad_region=6280, passed=55027
Got 55027 stars (including 46339 good ones) from the SExtractor catalog wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits.wcscat
util/solve_plate_with_UCAC5 got 55027 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.1'
Seting catalog search parameters based on the expected field of view 938.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013029 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010423 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.1 to 51.3)
Done reading UCAC5 zone files...
Matched 4932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4908 matched stars entering correct_measured_positions(), 4909 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4908 matched stars entering correct_measured_positions(), 50499 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
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 650 to 708 (Dec 40.1 to 51.3)
Done reading UCAC5 zone files...
Matched 4932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4906 matched stars entering correct_measured_positions(), 50499 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Accuracy estimation diagnostic: 4906 matched stars entering correct_measured_positions(), 50499 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 4906 stars left (next iteration limit 5398)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.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=4906 robust_rms=5.628 arcsec worst_quadrant_rms=14.125 arcsec
SIP_REFIT: SIP order 3 trial: matched=4906 robust_rms=0.653 arcsec worst_quadrant_rms=0.765 arcsec
SIP_REFIT: SIP order 5 trial: matched=4906 robust_rms=0.490 arcsec worst_quadrant_rms=0.536 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4906 robust_rms_before=0.959 arcsec robust_rms_before_corrected=0.496 arcsec robust_rms_after=0.490 arcsec worst_quadrant_rms_before=0.554 worst_quadrant_rms_after=0.536
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.554 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits N_match=4906 sigma_overall_arcsec=0.503 sigma_q1_arcsec=0.479 sigma_q2_arcsec=0.520 sigma_q3_arcsec=0.555 sigma_q4_arcsec=0.462 n_q1=1762 n_q2=669 n_q3=1667 n_q4=808 worst_quadrant_to_overall_ratio=1.104
The image catalog is written to wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits -region wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.MqJNrySJZh (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_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.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_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits
WCS_IMAGE_NAME=wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits
WCS-calibrated image found: wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits
Checking if the catalog wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits.wcscat corresponding to the image wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits.wcscat corresponding to the image wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits
WCS catalog name: wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=2626, bad_region=6298, passed=55666
Got 55666 stars (including 46920 good ones) from the SExtractor catalog wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits.wcscat
util/solve_plate_with_UCAC5 got 55666 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.1'
Seting catalog search parameters based on the expected field of view 938.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013029 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010423 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 650 to 708 (Dec 40.1 to 51.3)
Done reading UCAC5 zone files...
Matched 4934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4912 matched stars entering correct_measured_positions(), 4912 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4912 matched stars entering correct_measured_positions(), 51167 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
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 650 to 708 (Dec 40.1 to 51.3)
Done reading UCAC5 zone files...
Matched 4934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4913 matched stars entering correct_measured_positions(), 51167 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.46"
Accuracy estimation diagnostic: 4913 matched stars entering correct_measured_positions(), 51167 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 4913 stars left (next iteration limit 5403)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.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=4913 robust_rms=5.717 arcsec worst_quadrant_rms=13.204 arcsec
SIP_REFIT: SIP order 3 trial: matched=4913 robust_rms=0.638 arcsec worst_quadrant_rms=0.729 arcsec
SIP_REFIT: SIP order 5 trial: matched=4913 robust_rms=0.497 arcsec worst_quadrant_rms=0.550 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4913 robust_rms_before=0.934 arcsec robust_rms_before_corrected=0.502 arcsec robust_rms_after=0.497 arcsec worst_quadrant_rms_before=0.557 worst_quadrant_rms_after=0.550
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.557 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits N_match=4913 sigma_overall_arcsec=0.520 sigma_q1_arcsec=0.491 sigma_q2_arcsec=0.553 sigma_q3_arcsec=0.594 sigma_q4_arcsec=0.466 n_q1=1771 n_q2=683 n_q3=1645 n_q4=814 worst_quadrant_to_overall_ratio=1.142
The image catalog is written to wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits -region wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
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_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.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_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-18_20.00sec_-0.00C_LIGHT_0131.fits
Saving fully-calibrated image wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.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_2026-08-25_CI_Per-02-Q2b1x1_012439_TTUQ2b1x1_2820299_9Rv8d46J/wcs_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132.fits
Preparing the HTML report for the field Per-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:04:18.94 +45:53:22.5: 12.71 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:41:09.47 +47:11:18.3: 12.11 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:08:20.94 +46:10:58.7: 12.88 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:41:09.47 +47:11:18.3: 12.11 +/- 0.01 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:04:18.94 +45:53:22.5: 12.71 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:08:20.94 +46:10:58.7: 12.79 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.71 +/- 0.01
Forced photometry reference-image weighted average: 12.11 +/- 0.01
Forced photometry filter REJECTED candidate at 03:04:18.94 +45:53:22.5: ref_mag=12.71 +/- 0.01 new_mean_mag=12.9377 delta=-0.23 (need > 0.90)
Forced photometry filter REJECTED candidate at 03:41:09.47 +47:11:18.3: ref_mag=12.11 +/- 0.01 new_mean_mag=12.2745 delta=-0.17 (need > 0.90)
Forced photometry reference-image weighted average: 12.83 +/- 0.01
Forced photometry filter REJECTED candidate at 03:08:20.94 +46:10:58.7: ref_mag=12.83 +/- 0.01 new_mean_mag=12.9673 delta=-0.14 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:13:58.76 +43:53:01.0: 12.98 +/- 0.02 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:13:58.76 +43:53:01.0: 12.99 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.99 +/- 0.02
Forced photometry filter REJECTED candidate at 03:13:58.76 +43:53:01.0: ref_mag=12.99 +/- 0.02 new_mean_mag=12.8512 delta=0.13 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:23:02.05 +44:57:22.2: 13.66 +/- 0.04 detection
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-07_20.00sec_-15.00C_LIGHT_0020.fits at 03:02:41.30 +41:33:40.5: 15.99 +/- 99.00 upperlimit
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:23:02.05 +44:57:22.2: 13.66 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.66 +/- 0.03
Forced photometry filter REJECTED candidate at 03:23:02.05 +44:57:22.2: ref_mag=13.66 +/- 0.03 new_mean_mag=13.2757 delta=0.39 (need > 0.90)
Forced photometry on wcs_Per-02-Q2b1x1_2026-01-08_19-58-49_20.00sec_-15.00C_LIGHT_0021.fits at 03:02:41.30 +41:33:40.5: 15.99 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out213160.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 54s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 212364_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 212364_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:21:22.37 +45:38:40.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212378_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 212378_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:53:46.86 +48:40:46.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212379_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 212379_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
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Considering the candidate 212392_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 212392_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
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Considering the candidate 212393_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 212393_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:51:50.07 +43:39:59.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212395_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 212395_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:00:47.62 +48:34:02.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212396_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 212396_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:13:53.65 +43:50:14.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212399_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 212399_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:32:59.44 +43:43:57.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212401_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 212401_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
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Considering the candidate 212468_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 212468_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 212490_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 212490_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 212514_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 212514_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:09:13.95 +44:50:34.2 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 212534_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 212534_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 212551_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 212551_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:53:30.06 +47:39:01.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212596_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 212596_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:01:38.26 +42:41:28.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212639_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 212639_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 212656_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 212656_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:23:02.54 +49:13:28.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 212668_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 212668_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:44:45.09 +46:07:13.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 212683_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 212683_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
**** FOUND 02:55:34.30 +48:21:27.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212705_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 212705_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:30:26.01 +48:06:29.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 212708_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 212708_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:17:45.85 +43:59:58.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 212720_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 212720_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:21:50.63 +49:05:44.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 212722_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 212722_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:51:30.29 +45:27:31.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212730_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 212730_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:28:44.07 +49:51:12.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 212759_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 212759_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:44:07.82 +47:27:17.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212767_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 212767_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:28:21.21 +44:21:11.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212773_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 212773_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
**** FOUND 02:59:47.23 +47:14:53.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 212781_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 212781_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
**** FOUND 02:57:48.39 +46:39:04.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212790_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 212790_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:46:04.36 +45:42:23.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 212802_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 212802_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:13:55.68 +43:53:23.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212812_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 212812_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
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Considering the candidate 212819_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 212819_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:23:19.79 +49:13:42.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 212846_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 212846_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 212885_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 212885_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:18:34.01 +44:41:59.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212891_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 212891_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:45:07.96 +48:28:00.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212901_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 212901_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:40:50.50 +43:41:42.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212908_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 212908_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:47:06.66 +46:37:10.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212920_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 212920_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:30:43.63 +48:01:37.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212924_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 212924_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:31:48.87 +48:45:24.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 212935_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 212935_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:19:15.98 +50:06:46.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 212938_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 212938_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:12:35.08 +47:44:42.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 212980_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 212980_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:13:28.30 +48:12:27.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 212998_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 212998_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:26:04.72 +49:46:25.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213039_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 213039_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:09:21.78 +45:39:32.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213057_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 213057_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:19:25.99 +44:00:33.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213086_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 213086_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:43:40.45 +42:35:49.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213092_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 213092_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
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Considering the candidate 213097_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 213097_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:51:28.35 +49:46:36.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213109_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 213109_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:56:05.47 +47:51:21.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 213127_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 213127_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 213138_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 213138_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:40:11.19 +44:14:52.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213145_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 213145_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:22:42.21 +41:56:32.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213146_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 213146_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:27:13.02 +48:12:15.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213160_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
Preparing report for the candidate 213160_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
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Considering the candidate 213162_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 213162_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 213169_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 213169_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:38:08.34 +48:14:46.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 213173_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 213173_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 166395_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 166395_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:42:34.75 +50:15:58.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 54778_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
Preparing report for the candidate 54778_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62475_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 62475_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:57:00.42 +44:32:05.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 128521_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 128521_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:26:29.66 +47:31:47.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 201415_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 201415_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:18:28.07 +42:49:19.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 145807_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 145807_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:54:56.57 +48:36:00.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 48255_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 48255_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
**** FOUND 03:37:25.18 +43:39:08.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 52260_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 52260_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 66312_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132
The candidate 66312_fd_Per-02-Q2b1x1_2026-08-25_01-23-58_20.00sec_-0.00C_LIGHT_0132 did not pass the final checks