This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 09 28.4278 2461311.9278 8.54 00:19:32.71 +08:37:53.0
109.62950 -53.41463 galactic Psc Second-epoch detections are separated by 0.8" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.192 Nausikaa -0 0 0 8.4 -0 -0
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits at 00:19:32.71 +08:37:53.0: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits at 00:19:32.71 +08:37:53.0: 15.70 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461311.9278,8.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260928.4278 8.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 28.4278 2461311.9278 13.54 00:19:28.05 +07:34:37.9
109.22167 -54.44129 galactic Psc Second-epoch detections are separated by 0.5" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.577 Rhea -0 -0 0 13.4 -0 -0
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits at 00:19:28.05 +07:34:37.9: 15.91 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits at 00:19:28.05 +07:34:37.9: 15.87 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461311.9278,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260928.4278 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 28.4278 2461311.9278 13.56 00:01:49.65 +10:00:37.1
103.30982 -50.96159 galactic Psc Second-epoch detections are separated by 1.2" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.701 Oriola -0 0 0 13.7 0 0
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits at 00:01:49.65 +10:00:37.1: 15.87 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits at 00:01:49.65 +10:00:37.1: 15.90 +/- 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461311.9278,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260928.4278 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461242.90183583 21.07.2026 09:38:28.616 /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
First image: 2461242.90183583 21.07.2026 09:38:28.616 /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
Last image: 2461311.92811817 28.09.2026 10:16:19.410 /data_ssd/NMW-TexasTech/workdir//img_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.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.: -7.31
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 2 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 5792
Objects passed selection criteria: 5778
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: 4206.75
Average stars matched: 4057 (96.4402 %)
Memory usage VmPeak: 232524 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Sep 25 15:05:03 CDT 2026
VaST build number 1.0rc89-225-g3a72982a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-25)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Sep 28 05:18:47 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461242.90183583 21.07.2026 09:38:28.616 /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
First image: 2461242.90183583 21.07.2026 09:38:28.616 /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
Last image: 2461311.92811817 28.09.2026 10:16:19.410 /data_ssd/NMW-TexasTech/workdir//img_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 21
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.05
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: 10 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): 30459
Objects passed selection criteria: 30394
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 24405.5
Average stars matched: 23460.5 (96.1279 %)
Memory usage VmPeak: 255052 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Sep 25 15:05:03 CDT 2026
VaST build number 1.0rc89-225-g3a72982a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-25)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Sep 28 05:19:36 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits
SExtractor catalog cache: saved Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits.cat to cache
SExtractor catalog cache: saved Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.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/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits
Checking WCS cache directory local_wcs_cache
Checking 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: 2461311.92749458
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_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits exists and is non-empty
wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits exists and is non-empty
wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits exists and is non-empty
wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits (1st reference image)
verification OK: wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
Image size: 937.3'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:59:58.228 +05:59:38.82 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits (1st new image)
verification OK: wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits
Image size: 941.7'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:00:03.772 +06:01:28.30 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 23:59:58.228 +05:59:38.82
Second-epoch image center 00:00:03.772 +06:01:28.30
Angular distance between the image centers 0.0381 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits (2nd new image)
verification OK: wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits
Image size: 941.7'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:00:05.782 +06:01:32.57 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:59:58.228 +05:59:38.82
Second-epoch image center 00:00:05.782 +06:01:32.57
Angular distance between the image centers 0.0445 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 00:00:03.772 +06:01:28.30
Second-epoch second image center 00:00:05.782 +06:01:32.57
Angular distance between the image centers 0.00841 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/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits &> /tmp/tmp.S7xmXJmDRN
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits &> /tmp/tmp.5RUcA6nICn
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits &> /tmp/tmp.N2y0MiSObW
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits &> /tmp/tmp.UiUGEsMY8n
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.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_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits and wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.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_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits and wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits.wcscat
Found non-empty wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits and wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits.wcscat
The reference image (wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits) and catalog (wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits.wcscat) found
'wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits.wcscat' -> 'wcsmag.cat'
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 6233 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 352.0271 to 7.9045 deg, Dec +0.6902 to +11.2647 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 352.0271 to 7.9045 deg, Dec 0.6902 to 11.2647 deg
Loaded 4566 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): 3722 out of 3826 total matches.
Matched with Tycho-2 3826 out of 6233 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.662650
a=0.000000 b=1.000000 c=22.662650
From vast_summary.log: estimated ref. image limiting mag.: -7.31
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.35
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.35
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 6233 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 352.0271 to 7.9045 deg, Dec +0.6902 to +11.2647 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 352.0271 to 7.9045 deg, Dec 0.6902 to 11.2647 deg
Loaded 4566 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): 3722 out of 3826 total matches.
Matched with Tycho-2 3826 out of 6233 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
Forced-photometry filter: calibrated wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits -> calib.txt_param_ref_wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits (aperture=6.4)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 6318 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 351.8996 to 8.2591 deg, Dec +0.3478 to +11.6137 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 351.8996 to 8.2591 deg, Dec 0.3478 to 11.6137 deg
Loaded 4984 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): 3763 out of 3845 total matches.
Matched with Tycho-2 3845 out of 6318 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits
Forced-photometry filter: calibrated wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits -> calib.txt_param_ref_wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits (aperture=6.2)
____ 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:
2.3 pix Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
2.4 pix Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits
2.2 pix fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits
2.2 pix fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits
Limiting magnitude estimates:
15.3 mag. Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
15.4 mag. Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits
14.2 mag. fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits
14.2 mag. fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits
All-image limiting magnitude estimate: 14.2 (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.S7xmXJmDRN (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/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.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_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits' -> 'wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.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/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
WCS_IMAGE_NAME=wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
WCS-calibrated image found: wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
Checking if the catalog wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits.wcscat corresponding to the image wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits alredy exist and is non-empty...
Catalog wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits.wcscat corresponding to the image wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
WCS catalog name: wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=357, bad_region=0, passed=6233
Got 6233 stars (including 5867 good ones) from the SExtractor catalog wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits.wcscat
util/solve_plate_with_UCAC5 got 6233 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 352.0271 through 0 to 7.9045, gap 7.9045 to 352.0271
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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4906 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4897 matched stars entering correct_measured_positions(), 4897 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4897 matched stars entering correct_measured_positions(), 6233 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 352.0274 through 0 to 7.9045, gap 7.9045 to 352.0274
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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4906 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4897 matched stars entering correct_measured_positions(), 6233 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4897 matched stars entering correct_measured_positions(), 6233 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 4897 stars left (next iteration limit 5386)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits N_match=4897 sigma_overall_arcsec=0.375 sigma_q1_arcsec=0.294 sigma_q2_arcsec=0.420 sigma_q3_arcsec=0.409 sigma_q4_arcsec=0.391 n_q1=1279 n_q2=1239 n_q3=1222 n_q4=1157 worst_quadrant_to_overall_ratio=1.120
The image catalog is written to wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits -region wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.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.5RUcA6nICn (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits' -> 'wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.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/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits
WCS_IMAGE_NAME=wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits
WCS-calibrated image found: wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits
Checking if the catalog wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits.wcscat corresponding to the image wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits alredy exist and is non-empty...
Catalog wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits.wcscat corresponding to the image wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits
WCS catalog name: wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=328, bad_region=0, passed=6318
Got 6318 stars (including 5982 good ones) from the SExtractor catalog wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits.wcscat
util/solve_plate_with_UCAC5 got 6318 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.8996 through 0 to 8.2591, gap 8.2591 to 351.8996
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 451 to 510 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 4903 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4892 matched stars entering correct_measured_positions(), 4892 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4892 matched stars entering correct_measured_positions(), 6318 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.8998 through 0 to 8.2592, gap 8.2592 to 351.8998
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 451 to 510 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 4903 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4892 matched stars entering correct_measured_positions(), 6318 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4892 matched stars entering correct_measured_positions(), 6318 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 4892 stars left (next iteration limit 5381)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits N_match=4892 sigma_overall_arcsec=0.303 sigma_q1_arcsec=0.271 sigma_q2_arcsec=0.326 sigma_q3_arcsec=0.300 sigma_q4_arcsec=0.304 n_q1=1292 n_q2=1193 n_q3=1278 n_q4=1129 worst_quadrant_to_overall_ratio=1.077
The image catalog is written to wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits -region wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.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.N2y0MiSObW (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_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.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_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits
WCS_IMAGE_NAME=wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits
WCS-calibrated image found: wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits
Checking if the catalog wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits.wcscat corresponding to the image wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits.wcscat corresponding to the image wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits
WCS catalog name: wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=309, bad_region=0, passed=2205
Got 2205 stars (including 1894 good ones) from the SExtractor catalog wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits.wcscat
util/solve_plate_with_UCAC5 got 2205 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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
RA wraps around 0/360 boundary: field RA 351.9005 through 0 to 8.2227, gap 8.2227 to 351.9005
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 451 to 509 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 1851 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1848 matched stars entering correct_measured_positions(), 1848 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1848 matched stars entering correct_measured_positions(), 2205 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
RA wraps around 0/360 boundary: field RA 351.9001 through 0 to 8.2230, gap 8.2230 to 351.9001
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 451 to 509 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 1851 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1848 matched stars entering correct_measured_positions(), 2205 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 1848 matched stars entering correct_measured_positions(), 2205 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 1848 stars left (next iteration limit 2032)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=1848 robust_rms=13.291 arcsec worst_region_rms=23.956 arcsec outer_annulus_rms=23.956 arcsec
SIP_REFIT: SIP order 3 trial: matched=1848 robust_rms=0.595 arcsec worst_region_rms=0.670 arcsec outer_annulus_rms=0.670 arcsec
SIP_REFIT: SIP order 5 trial: matched=1848 robust_rms=0.401 arcsec worst_region_rms=0.446 arcsec outer_annulus_rms=0.425 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=1848 robust_rms_before=1.029 arcsec robust_rms_before_corrected=0.362 arcsec robust_rms_after=0.401 arcsec worst_region_rms_before=0.407 worst_region_rms_after=0.446 outer_annulus_rms_before=1.082 outer_annulus_rms_after=0.425
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.407 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits worst_region_rms_kept=0.407 arcsec robust_rms_kept=0.362 arcsec matched=1848
WCS_QUALITY_DIAG: file=fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits N_match=1848 sigma_overall_arcsec=0.361 sigma_q1_arcsec=0.342 sigma_q2_arcsec=0.424 sigma_q3_arcsec=0.324 sigma_q4_arcsec=0.377 n_q1=419 n_q2=458 n_q3=480 n_q4=491 worst_quadrant_to_overall_ratio=1.175
The image catalog is written to wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits -region wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.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.UiUGEsMY8n (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_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.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_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits
WCS_IMAGE_NAME=wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits
WCS-calibrated image found: wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits
Checking if the catalog wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits.wcscat corresponding to the image wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits.wcscat corresponding to the image wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits
WCS catalog name: wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=327, bad_region=0, passed=2168
Got 2168 stars (including 1839 good ones) from the SExtractor catalog wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits.wcscat
util/solve_plate_with_UCAC5 got 2168 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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
RA wraps around 0/360 boundary: field RA 351.9007 through 0 to 8.2225, gap 8.2225 to 351.9007
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 451 to 509 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 1797 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1793 matched stars entering correct_measured_positions(), 1793 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 1793 matched stars entering correct_measured_positions(), 2168 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.9001 through 0 to 8.2229, gap 8.2229 to 351.9001
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 451 to 509 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 1797 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 1793 matched stars entering correct_measured_positions(), 2168 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 1793 matched stars entering correct_measured_positions(), 2168 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 1793 stars left (next iteration limit 1972)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=1793 robust_rms=13.524 arcsec worst_region_rms=23.412 arcsec outer_annulus_rms=23.412 arcsec
SIP_REFIT: SIP order 3 trial: matched=1793 robust_rms=0.684 arcsec worst_region_rms=0.761 arcsec outer_annulus_rms=0.761 arcsec
SIP_REFIT: SIP order 5 trial: matched=1793 robust_rms=0.438 arcsec worst_region_rms=0.460 arcsec outer_annulus_rms=0.417 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=1793 robust_rms_before=1.057 arcsec robust_rms_before_corrected=0.384 arcsec robust_rms_after=0.438 arcsec worst_region_rms_before=0.444 worst_region_rms_after=0.460 outer_annulus_rms_before=1.081 outer_annulus_rms_after=0.417
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.444 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits worst_region_rms_kept=0.444 arcsec robust_rms_kept=0.384 arcsec matched=1793
WCS_QUALITY_DIAG: file=fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits N_match=1793 sigma_overall_arcsec=0.381 sigma_q1_arcsec=0.344 sigma_q2_arcsec=0.464 sigma_q3_arcsec=0.362 sigma_q4_arcsec=0.376 n_q1=397 n_q2=451 n_q3=459 n_q4=486 worst_quadrant_to_overall_ratio=1.219
The image catalog is written to wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits -region wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.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_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits to local_wcs_cache/
'wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits' -> 'local_wcs_cache/wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits'
Saving the final (post-refit) wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits to local_wcs_cache/
'wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits' -> 'local_wcs_cache/wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits'
Saving the final (post-refit) wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits to local_wcs_cache/
'wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits' -> 'local_wcs_cache/wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits'
Saving the final (post-refit) wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits to local_wcs_cache/
'wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits' -> 'local_wcs_cache/wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits sigma_overall=0.375 worst_q_ratio=1.120
ref2=Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits sigma_overall=0.303 worst_q_ratio=1.077
new1=fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits sigma_overall=0.361 worst_q_ratio=1.175
new2=fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits sigma_overall=0.381 worst_q_ratio=1.219
reference average sigma_overall=0.339 worst_q_ratio=1.0985
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966_astrometric_residuals.png (4897 matched stars from wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.32 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382_astrometric_residuals.png (4892 matched stars from wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444_astrometric_residuals.png (1848 matched stars from wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.33 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445_astrometric_residuals.png (1793 matched stars from wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.34 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits'
Saving fully-calibrated image wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits'
Preparing the HTML report for the field Psc-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits at 00:19:32.71 +08:37:53.0: 15.70 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits at 00:19:32.71 +08:37:53.0: 15.70 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out20592.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20592_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445
Preparing report for the candidate 20592_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20595_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445
The candidate 20595_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445 did not pass the final checks
**** FOUND 23:36:10.41 +09:48:57.1 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 7s
Prepared the HTML report for the field Psc-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
00:19:32.71 +08:37:53.0
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/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits
SExtractor catalog cache: saved Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits.cat to cache
SExtractor catalog cache: saved Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
Creating symlink local_wcs_cache/wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits
Checking 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_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits exists and is non-empty
wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits exists and is non-empty
wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits exists and is non-empty
wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits (1st reference image)
verification OK: wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
Image size: 937.3'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:59:58.228 +05:59:38.82 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits (1st new image)
verification OK: wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits
Image size: 941.7'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:00:03.772 +06:01:28.30 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 23:59:58.228 +05:59:38.82
Second-epoch image center 00:00:03.772 +06:01:28.30
Angular distance between the image centers 0.0381 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits (2nd new image)
verification OK: wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits
Image size: 941.7'x626.9' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 00:00:05.782 +06:01:32.57 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 23:59:58.228 +05:59:38.82
Second-epoch image center 00:00:05.782 +06:01:32.57
Angular distance between the image centers 0.0445 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 00:00:03.772 +06:01:28.30
Second-epoch second image center 00:00:05.782 +06:01:32.57
Angular distance between the image centers 0.00841 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/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits &> /tmp/tmp.8Z5V4rn2vb
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits &> /tmp/tmp.6W4VpEEGAD
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits &> /tmp/tmp.d0W2aFUH8J
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits &> /tmp/tmp.RpJzQMFIYC
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.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_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits and wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.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_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits and wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits.wcscat
Found non-empty wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits and wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits.wcscat
The reference image (wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits) and catalog (wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits.wcscat) found
'wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits.wcscat' -> 'wcsmag.cat'
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 33634 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 351.9992 to 7.9160 deg, Dec +0.6902 to +11.2656 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 351.9992 to 7.9160 deg, Dec 0.6902 to 11.2656 deg
Loaded 4573 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): 3677 out of 3960 total matches.
Matched with Tycho-2 3960 out of 33634 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.546200
a=0.000000 b=1.000000 c=22.546200
From vast_summary.log: estimated ref. image limiting mag.: -7.05
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.50
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.50
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 33634 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 351.9992 to 7.9160 deg, Dec +0.6902 to +11.2656 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 351.9992 to 7.9160 deg, Dec 0.6902 to 11.2656 deg
Loaded 4573 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): 3677 out of 3960 total matches.
Matched with Tycho-2 3960 out of 33634 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
Forced-photometry filter: calibrated wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits -> calib.txt_param_ref_wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits (aperture=5.0)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 33762 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 351.8996 to 8.2739 deg, Dec +0.3067 to +11.6461 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 351.8996 to 8.2739 deg, Dec 0.3067 to 11.6461 deg
Loaded 5018 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): 3715 out of 3975 total matches.
Matched with Tycho-2 3975 out of 33762 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits
Forced-photometry filter: calibrated wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits -> calib.txt_param_ref_wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits (aperture=5.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 21 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.1 pix Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
2.4 pix Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits
2.0 pix fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits
1.9 pix fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits
Limiting magnitude estimates:
15.5 mag. Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
15.5 mag. Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits
14.2 mag. fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits
14.3 mag. fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits
All-image limiting magnitude estimate: 14.2 (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.8Z5V4rn2vb (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/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.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_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits' -> 'wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.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/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
WCS_IMAGE_NAME=wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
WCS-calibrated image found: wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
Checking if the catalog wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits.wcscat corresponding to the image wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits alredy exist and is non-empty...
Catalog wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits.wcscat corresponding to the image wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits
WCS catalog name: wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=22, blended=1340, bad_region=0, passed=33612
Got 33612 stars (including 32227 good ones) from the SExtractor catalog wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits.wcscat
util/solve_plate_with_UCAC5 got 33612 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.9992 through 0 to 7.9160, gap 7.9160 to 351.9992
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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4899 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4893 matched stars entering correct_measured_positions(), 4893 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4893 matched stars entering correct_measured_positions(), 33612 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.9998 through 0 to 7.9160, gap 7.9160 to 351.9998
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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 4899 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4893 matched stars entering correct_measured_positions(), 33612 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4893 matched stars entering correct_measured_positions(), 33612 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 4893 stars left (next iteration limit 5382)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.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_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits N_match=4893 sigma_overall_arcsec=0.364 sigma_q1_arcsec=0.285 sigma_q2_arcsec=0.406 sigma_q3_arcsec=0.403 sigma_q4_arcsec=0.369 n_q1=1276 n_q2=1249 n_q3=1197 n_q4=1171 worst_quadrant_to_overall_ratio=1.116
The image catalog is written to wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits -region wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.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.6W4VpEEGAD (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits' -> 'wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.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/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits
WCS_IMAGE_NAME=wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits
WCS-calibrated image found: wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits
Checking if the catalog wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits.wcscat corresponding to the image wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits alredy exist and is non-empty...
Catalog wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits.wcscat corresponding to the image wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits
WCS catalog name: wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=1193, bad_region=21, passed=33746
Got 33746 stars (including 32487 good ones) from the SExtractor catalog wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits.wcscat
util/solve_plate_with_UCAC5 got 33746 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.2'
Seting catalog search parameters based on the expected field of view 941.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013072 (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 0.010458 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.8996 through 0 to 8.2739, gap 8.2739 to 351.8996
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 451 to 510 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 4895 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4885 matched stars entering correct_measured_positions(), 4885 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4885 matched stars entering correct_measured_positions(), 33746 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.8999 through 0 to 8.2739, gap 8.2739 to 351.8999
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 451 to 510 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 4895 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4885 matched stars entering correct_measured_positions(), 33746 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.26"
Accuracy estimation diagnostic: 4885 matched stars entering correct_measured_positions(), 33746 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 4885 stars left (next iteration limit 5373)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.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_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits N_match=4885 sigma_overall_arcsec=0.294 sigma_q1_arcsec=0.267 sigma_q2_arcsec=0.311 sigma_q3_arcsec=0.294 sigma_q4_arcsec=0.298 n_q1=1273 n_q2=1211 n_q3=1272 n_q4=1129 worst_quadrant_to_overall_ratio=1.059
The image catalog is written to wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits -region wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.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.d0W2aFUH8J (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_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.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_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits
WCS_IMAGE_NAME=wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits
WCS-calibrated image found: wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits
Checking if the catalog wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits.wcscat corresponding to the image wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits.wcscat corresponding to the image wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits
WCS catalog name: wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=2, no_mag_err=0, low_SNR=2, blended=457, bad_region=1, passed=15362
Got 15362 stars (including 14872 good ones) from the SExtractor catalog wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits.wcscat
util/solve_plate_with_UCAC5 got 15362 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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
RA wraps around 0/360 boundary: field RA 351.8717 through 0 to 8.2731, gap 8.2731 to 351.8717
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 451 to 510 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 4889 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4882 matched stars entering correct_measured_positions(), 4882 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4882 matched stars entering correct_measured_positions(), 15362 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.8714 through 0 to 8.2736, gap 8.2736 to 351.8714
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 451 to 510 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 4890 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4882 matched stars entering correct_measured_positions(), 15362 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 4882 matched stars entering correct_measured_positions(), 15362 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 4882 stars left (next iteration limit 5370)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.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=4882 robust_rms=13.029 arcsec worst_region_rms=27.895 arcsec outer_annulus_rms=27.895 arcsec
SIP_REFIT: SIP order 3 trial: matched=4882 robust_rms=0.634 arcsec worst_region_rms=0.784 arcsec outer_annulus_rms=0.784 arcsec
SIP_REFIT: SIP order 5 trial: matched=4882 robust_rms=0.460 arcsec worst_region_rms=0.516 arcsec outer_annulus_rms=0.490 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4882 robust_rms_before=1.043 arcsec robust_rms_before_corrected=0.390 arcsec robust_rms_after=0.460 arcsec worst_region_rms_before=0.442 worst_region_rms_after=0.516 outer_annulus_rms_before=1.173 outer_annulus_rms_after=0.490
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.442 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits worst_region_rms_kept=0.442 arcsec robust_rms_kept=0.390 arcsec matched=4882
WCS_QUALITY_DIAG: file=fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits N_match=4882 sigma_overall_arcsec=0.392 sigma_q1_arcsec=0.377 sigma_q2_arcsec=0.407 sigma_q3_arcsec=0.371 sigma_q4_arcsec=0.403 n_q1=1190 n_q2=1230 n_q3=1234 n_q4=1228 worst_quadrant_to_overall_ratio=1.038
The image catalog is written to wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits -region wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.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.RpJzQMFIYC (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_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.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_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits
WCS_IMAGE_NAME=wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits
WCS-calibrated image found: wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits
Checking if the catalog wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits.wcscat corresponding to the image wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits.wcscat corresponding to the image wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits
WCS catalog name: wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=1, no_mag_err=0, low_SNR=6, blended=459, bad_region=0, passed=15517
Got 15517 stars (including 15036 good ones) from the SExtractor catalog wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits.wcscat
util/solve_plate_with_UCAC5 got 15517 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (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 0.010463 (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
RA wraps around 0/360 boundary: field RA 351.8714 through 0 to 8.2618, gap 8.2618 to 351.8714
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 451 to 510 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 4892 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4884 matched stars entering correct_measured_positions(), 4884 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4884 matched stars entering correct_measured_positions(), 15517 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 351.8708 through 0 to 8.2625, gap 8.2625 to 351.8708
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 451 to 510 (Dec 0.3 to 11.6)
Done reading UCAC5 zone files...
Matched 4893 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4884 matched stars entering correct_measured_positions(), 15517 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 4884 matched stars entering correct_measured_positions(), 15517 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 4884 stars left (next iteration limit 5372)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.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=4884 robust_rms=13.280 arcsec worst_region_rms=27.681 arcsec outer_annulus_rms=27.681 arcsec
SIP_REFIT: SIP order 3 trial: matched=4884 robust_rms=0.723 arcsec worst_region_rms=0.844 arcsec outer_annulus_rms=0.844 arcsec
SIP_REFIT: SIP order 5 trial: matched=4884 robust_rms=0.489 arcsec worst_region_rms=0.508 arcsec outer_annulus_rms=0.486 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4884 robust_rms_before=1.076 arcsec robust_rms_before_corrected=0.426 arcsec robust_rms_after=0.489 arcsec worst_region_rms_before=0.461 worst_region_rms_after=0.508 outer_annulus_rms_before=1.157 outer_annulus_rms_after=0.486
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.461 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits worst_region_rms_kept=0.461 arcsec robust_rms_kept=0.426 arcsec matched=4884
WCS_QUALITY_DIAG: file=fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits N_match=4884 sigma_overall_arcsec=0.422 sigma_q1_arcsec=0.419 sigma_q2_arcsec=0.451 sigma_q3_arcsec=0.394 sigma_q4_arcsec=0.409 n_q1=1184 n_q2=1233 n_q3=1239 n_q4=1228 worst_quadrant_to_overall_ratio=1.069
The image catalog is written to wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits -region wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.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_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.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_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-15-25_20.00sec_-0.00C_LIGHTs_0444.fits
Saving fully-calibrated image wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.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_2026-09-28_CI_Psc-04-Q1b1x1_051713_TTUQ1b1x1_865379_aX3cXGAH/wcs_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445.fits
Preparing the HTML report for the field Psc-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits at 00:08:34.50 +01:53:59.6: 12.71 +/- 0.02 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits at 00:00:59.47 +07:09:39.5: 12.20 +/- 0.01 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits at 00:04:06.09 +11:05:06.2: 12.90 +/- 0.02 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits at 23:55:38.93 +08:45:56.6: 11.49 +/- 0.01 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits at 23:40:48.61 +10:28:17.9: 12.32 +/- 0.02 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits at 00:23:37.45 +04:58:27.0: 13.05 +/- 0.03 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits at 00:26:52.06 +09:18:19.4: 12.86 +/- 0.03 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits at 00:02:24.34 +08:23:08.0: 13.10 +/- 0.03 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits at 00:08:34.50 +01:53:59.6: 12.72 +/- 0.02 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits at 00:23:37.45 +04:58:27.0: 13.08 +/- 0.03 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits at 23:55:38.93 +08:45:56.6: 11.70 +/- 0.01 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits at 00:04:06.09 +11:05:06.2: 12.86 +/- 0.02 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits at 23:40:48.61 +10:28:17.9: 12.33 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.72 +/- 0.01
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits at 23:51:51.89 +07:28:01.6: 13.34 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.02
Forced photometry reference-image weighted average: 12.88 +/- 0.02
Forced photometry reference-image weighted average: 11.58 +/- 0.00
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits at 00:00:59.47 +07:09:39.5: 12.26 +/- 0.01 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits at 00:19:28.05 +07:34:37.9: 15.91 +/- 99.00 upperlimit
Forced photometry filter REJECTED candidate at 00:08:34.50 +01:53:59.6: ref_mag=12.72 +/- 0.01 new_mean_mag=13.1480 delta=-0.43 (need > 0.90)
Forced photometry reference-image weighted average: 12.33 +/- 0.01
Forced photometry filter REJECTED candidate at 00:23:37.45 +04:58:27.0: ref_mag=13.07 +/- 0.02 new_mean_mag=13.2887 delta=-0.22 (need > 0.90)
Forced photometry filter REJECTED candidate at 00:04:06.09 +11:05:06.2: ref_mag=12.88 +/- 0.02 new_mean_mag=13.2618 delta=-0.38 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:55:38.93 +08:45:56.6: ref_mag=11.58 +/- 0.00 new_mean_mag=12.0048 delta=-0.42 (need > 0.90)
Forced photometry filter REJECTED candidate at 23:40:48.61 +10:28:17.9: ref_mag=12.33 +/- 0.01 new_mean_mag=12.6759 delta=-0.35 (need > 0.90)
Forced photometry reference-image weighted average: 12.23 +/- 0.01
Forced photometry filter REJECTED candidate at 00:00:59.47 +07:09:39.5: ref_mag=12.23 +/- 0.01 new_mean_mag=12.6094 delta=-0.38 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits at 00:26:52.06 +09:18:19.4: 12.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.02
Forced photometry filter REJECTED candidate at 00:26:52.06 +09:18:19.4: ref_mag=12.75 +/- 0.02 new_mean_mag=12.9369 delta=-0.19 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits at 00:02:24.34 +08:23:08.0: 13.15 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.12 +/- 0.02
Forced photometry filter REJECTED candidate at 00:02:24.34 +08:23:08.0: ref_mag=13.12 +/- 0.02 new_mean_mag=13.3100 delta=-0.19 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits at 23:51:51.89 +07:28:01.6: 13.29 +/- 0.04 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits at 00:19:28.05 +07:34:37.9: 15.87 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.32 +/- 0.03
Forced photometry filter REJECTED candidate at 23:51:51.89 +07:28:01.6: ref_mag=13.32 +/- 0.03 new_mean_mag=13.4613 delta=-0.15 (need > 0.90)
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits at 23:51:50.36 +07:26:41.3: 13.52 +/- 0.05 detection
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-21_04-38-28_20.00sec_4.90C_LIGHT_0966.fits at 00:01:49.65 +10:00:37.1: 15.87 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits at 00:01:49.65 +10:00:37.1: 15.90 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-04-Q1b1x1_2026-07-22_04-54-46_20.00sec_0.00C_LIGHTs_0382.fits at 23:51:50.36 +07:26:41.3: 13.49 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.50 +/- 0.03
Forced photometry filter REJECTED candidate at 23:51:50.36 +07:26:41.3: ref_mag=13.50 +/- 0.03 new_mean_mag=13.5286 delta=-0.03 (need > 0.90)
Adding exclusion_list_local.txt__out53740.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53746.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 53677_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445
The candidate 53677_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53678_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445
The candidate 53678_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53679_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445
The candidate 53679_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53680_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445
The candidate 53680_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53681_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445
The candidate 53681_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445 did not pass the final checks
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Considering the candidate 53682_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445
The candidate 53682_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53684_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445
The candidate 53684_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445 did not pass the final checks
**** FOUND 00:19:32.72 +08:37:53.2 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53707_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445
The candidate 53707_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445 did not pass the final checks
**** FOUND 23:42:00.72 +01:48:29.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53708_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445
The candidate 53708_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445 did not pass the final checks
**** FOUND 23:51:22.71 +09:20:49.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 53715_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445
The candidate 53715_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445 did not pass the final checks
**** FOUND 00:25:29.92 +01:56:52.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 53723_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445
The candidate 53723_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445 did not pass the final checks
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Considering the candidate 53730_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445
The candidate 53730_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445 did not pass the final checks
Rejecting candidate due to large distance (29.8") between the two second-epoch detections
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Considering the candidate 53734_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445
The candidate 53734_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445 did not pass the final checks
Rejecting candidate due to large distance (29.2") between the two second-epoch detections
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Considering the candidate 53735_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445
The candidate 53735_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445 did not pass the final checks
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Considering the candidate 53740_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445
Preparing report for the candidate 53740_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445
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Considering the candidate 53742_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445
The candidate 53742_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445 did not pass the final checks
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Considering the candidate 53746_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445
Preparing report for the candidate 53746_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445
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Considering the candidate 53747_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445
The candidate 53747_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445 did not pass the final checks
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Considering the candidate 53748_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445
The candidate 53748_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445 did not pass the final checks
Rejecting candidate due to large distance (28.2") between the two second-epoch detections
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Considering the candidate 53749_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445
The candidate 53749_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445 did not pass the final checks
Rejecting candidate due to large distance (29.0") between the two second-epoch detections
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Considering the candidate 26495_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445
The candidate 26495_fd_Psc-04-Q1b1x1_2026-09-28_05-16-19_20.00sec_0.00C_LIGHTs_0445 did not pass the final checks