This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX
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 12.4127 2461295.9127 12.25 03:06:00.85 +02:01:09.3
176.36376 -46.41765 galactic Cet Second-epoch detections are separated by 0.4" and 10.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.129 Antigone -0 -0 0 12.6 -0 -0
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 03:06:00.85 +02:01:09.3: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 03:06:00.85 +02:01:09.3: 15.82 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 12.4127* 03 06 00.85 +02 01 09.3 12.2 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461295.9127,12.25,0.05,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 20260912.4127 12.25CV 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 12.4127 2461295.9127 13.41 03:14:53.33 +03:09:45.0
177.37789 -44.02822 galactic Cet Second-epoch detections are separated by 0.8" and 10.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.464 Megaira -1 -0 1 13.5 0 0
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 03:14:53.33 +03:09:45.0: 15.99 +/- 99.00 upperlimit
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 03:14:53.33 +03:09:45.0: 16.00 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 09 12.4127* 03 14 53.33 +03 09 45.0 13.4 U Cet 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461295.9127,13.41,0.05,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 20260912.4127 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.65583366 09.01.2026 03:44:14.028 /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
First image: 2461049.65583366 09.01.2026 03:44:14.028 /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
Last image: 2461295.91307360 12.09.2026 09:54:39.559 /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 5
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.54
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 3
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 7574
Objects passed selection criteria: 7573
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 7190.75
Average stars matched: 6941.5 (96.5337 %)
Memory usage VmPeak: 233488 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Sep 11 14:55:52 CDT 2026
VaST build number 1.0rc89-210-g97d43bca
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Sep 12 05:09:08 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.65583366 09.01.2026 03:44:14.028 /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
First image: 2461049.65583366 09.01.2026 03:44:14.028 /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
Last image: 2461295.91307360 12.09.2026 09:54:39.559 /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 25
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.29
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: 32 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): 38148
Objects passed selection criteria: 38069
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 35987
Average stars matched: 34840.5 (96.8141 %)
Memory usage VmPeak: 259372 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Sep 11 14:55:52 CDT 2026
VaST build number 1.0rc89-210-g97d43bca
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Sep 12 05:11:57 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/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits
SExtractor catalog cache: saved Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits.cat to cache
SExtractor catalog cache: saved Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.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/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461295.91231890
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
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits exists and is non-empty
wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits exists and is non-empty
wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits exists and is non-empty
wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits (1st reference image)
verification OK: wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
Image size: 941.5'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 03:25:43.554 -02:00:23.97 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits (1st new image)
verification OK: wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits
Image size: 941.0'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 03:25:49.030 -01:57:18.59 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 03:25:43.554 -02:00:23.97
Second-epoch image center 03:25:49.030 -01:57:18.59
Angular distance between the image centers 0.0563 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits (2nd new image)
verification OK: wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits
Image size: 941.0'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 03:25:52.189 -01:57:58.26 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 03:25:43.554 -02:00:23.97
Second-epoch image center 03:25:52.189 -01:57:58.26
Angular distance between the image centers 0.0541 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 03:25:49.030 -01:57:18.59
Second-epoch second image center 03:25:52.189 -01:57:58.26
Angular distance between the image centers 0.01716 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/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits &> /tmp/tmp.dPWpvHDbMb
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits &> /tmp/tmp.iJpfyIZxAd
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits &> /tmp/tmp.6o1fqFYDO9
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits &> /tmp/tmp.HKg6SXLRHH
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits
Calibrating the magnitude scale
Found non-empty wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.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_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits and wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.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_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits and wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits.wcscat
Found non-empty wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits and wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits.wcscat
The reference image (wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits) and catalog (wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits.wcscat) found
'wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits.wcscat' -> 'wcsmag.cat'
Read 7165 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 43.5324 to 59.3891 deg, Dec -7.3136 to +3.3057 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 43.5324 to 59.3891 deg, Dec -7.3136 to 3.3057 deg
Loaded 4649 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): 3753 out of 3933 total matches.
Matched with Tycho-2 3933 out of 7165 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.908300
a=0.000000 b=1.000000 c=22.908300
From vast_summary.log: estimated ref. image limiting mag.: -7.54
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.37
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.37
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 7165 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 43.5324 to 59.3891 deg, Dec -7.3136 to +3.3057 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 43.5324 to 59.3891 deg, Dec -7.3136 to 3.3057 deg
Loaded 4649 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): 3753 out of 3933 total matches.
Matched with Tycho-2 3933 out of 7165 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
Forced-photometry filter: calibrated wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits -> calib.txt_param_ref_wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits (aperture=6.0)
Read 7098 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 43.5101 to 59.3815 deg, Dec -7.3136 to +3.3024 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 43.5101 to 59.3815 deg, Dec -7.3136 to 3.3024 deg
Loaded 4649 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): 3745 out of 3917 total matches.
Matched with Tycho-2 3917 out of 7098 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
Forced-photometry filter: calibrated wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits -> calib.txt_param_ref_wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits (aperture=6.0)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
2.0 pix Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
2.7 pix fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits
2.7 pix fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits
Limiting magnitude estimates:
15.4 mag. Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
15.4 mag. Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
15.2 mag. fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits
15.2 mag. fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits
All-image limiting magnitude estimate: 15.2 (SNR ) 12.2 (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.dPWpvHDbMb (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_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits' -> 'wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.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/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
WCS_IMAGE_NAME=wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
WCS-calibrated image found: wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
Checking if the catalog wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits.wcscat corresponding to the image wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits alredy exist and is non-empty...
Catalog wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits.wcscat corresponding to the image wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
WCS catalog name: wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.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=532, bad_region=0, passed=7165
Got 7165 stars (including 6616 good ones) from the SExtractor catalog wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits.wcscat
util/solve_plate_with_UCAC5 got 7165 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4897 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4894 matched stars entering correct_measured_positions(), 4894 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4894 matched stars entering correct_measured_positions(), 7165 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.22"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4897 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4894 matched stars entering correct_measured_positions(), 7165 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Accuracy estimation diagnostic: 4894 matched stars entering correct_measured_positions(), 7165 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Excluding outliers - 4894 stars left (next iteration limit 5383)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits N_match=4894 sigma_overall_arcsec=0.259 sigma_q1_arcsec=0.337 sigma_q2_arcsec=0.250 sigma_q3_arcsec=0.231 sigma_q4_arcsec=0.224 n_q1=1232 n_q2=1175 n_q3=1357 n_q4=1130 worst_quadrant_to_overall_ratio=1.300
The image catalog is written to wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits -region wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.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.iJpfyIZxAd (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_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits' -> 'wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.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/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
WCS_IMAGE_NAME=wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
WCS-calibrated image found: wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
Checking if the catalog wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits.wcscat corresponding to the image wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits alredy exist and is non-empty...
Catalog wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits.wcscat corresponding to the image wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
WCS catalog name: wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.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=523, bad_region=0, passed=7098
Got 7098 stars (including 6565 good ones) from the SExtractor catalog wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits.wcscat
util/solve_plate_with_UCAC5 got 7098 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4900 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4896 matched stars entering correct_measured_positions(), 4896 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4896 matched stars entering correct_measured_positions(), 7098 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.22"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4900 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4895 matched stars entering correct_measured_positions(), 7098 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Accuracy estimation diagnostic: 4895 matched stars entering correct_measured_positions(), 7098 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Excluding outliers - 4895 stars left (next iteration limit 5385)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits N_match=4895 sigma_overall_arcsec=0.263 sigma_q1_arcsec=0.343 sigma_q2_arcsec=0.255 sigma_q3_arcsec=0.237 sigma_q4_arcsec=0.230 n_q1=1233 n_q2=1170 n_q3=1359 n_q4=1133 worst_quadrant_to_overall_ratio=1.303
The image catalog is written to wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits -region wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.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.6o1fqFYDO9 (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_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.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_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits
WCS_IMAGE_NAME=wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits
WCS-calibrated image found: wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits
Checking if the catalog wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits.wcscat corresponding to the image wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits alredy exist and is non-empty...
Catalog wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits.wcscat corresponding to the image wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits
WCS catalog name: wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.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=394, bad_region=0, passed=7327
Got 7327 stars (including 6929 good ones) from the SExtractor catalog wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits.wcscat
util/solve_plate_with_UCAC5 got 7327 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 412 to 470 (Dec -7.5 to 3.7)
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: 4903 matched stars entering correct_measured_positions(), 4903 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4903 matched stars entering correct_measured_positions(), 7327 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 412 to 470 (Dec -7.5 to 3.7)
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: 4903 matched stars entering correct_measured_positions(), 7327 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Accuracy estimation diagnostic: 4903 matched stars entering correct_measured_positions(), 7327 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 4903 stars left (next iteration limit 5393)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4903 robust_rms=10.106 arcsec worst_quadrant_rms=10.403 arcsec
SIP_REFIT: SIP order 3 trial: matched=4903 robust_rms=0.345 arcsec worst_quadrant_rms=0.358 arcsec
SIP_REFIT: SIP order 5 trial: matched=4903 robust_rms=0.250 arcsec worst_quadrant_rms=0.269 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4903 robust_rms_before=0.936 arcsec robust_rms_before_corrected=0.255 arcsec robust_rms_after=0.250 arcsec worst_quadrant_rms_before=0.281 worst_quadrant_rms_after=0.269
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.281 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits N_match=4903 sigma_overall_arcsec=0.266 sigma_q1_arcsec=0.266 sigma_q2_arcsec=0.288 sigma_q3_arcsec=0.244 sigma_q4_arcsec=0.253 n_q1=1158 n_q2=1306 n_q3=1221 n_q4=1218 worst_quadrant_to_overall_ratio=1.082
The image catalog is written to wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits -region wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.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.HKg6SXLRHH (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_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.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_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits
WCS_IMAGE_NAME=wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits
WCS-calibrated image found: wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits
Checking if the catalog wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits.wcscat corresponding to the image wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits alredy exist and is non-empty...
Catalog wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits.wcscat corresponding to the image wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits
WCS catalog name: wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.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=394, bad_region=0, passed=7345
Got 7345 stars (including 6946 good ones) from the SExtractor catalog wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits.wcscat
util/solve_plate_with_UCAC5 got 7345 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 412 to 470 (Dec -7.5 to 3.7)
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: 4899 matched stars entering correct_measured_positions(), 4899 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.22"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4899 matched stars entering correct_measured_positions(), 7345 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.22"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 412 to 470 (Dec -7.5 to 3.7)
Done reading UCAC5 zone files...
Matched 4904 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4900 matched stars entering correct_measured_positions(), 7345 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Accuracy estimation diagnostic: 4900 matched stars entering correct_measured_positions(), 7345 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Excluding outliers - 4900 stars left (next iteration limit 5388)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4900 robust_rms=9.968 arcsec worst_quadrant_rms=10.265 arcsec
SIP_REFIT: SIP order 3 trial: matched=4900 robust_rms=0.316 arcsec worst_quadrant_rms=0.333 arcsec
SIP_REFIT: SIP order 5 trial: matched=4900 robust_rms=0.243 arcsec worst_quadrant_rms=0.277 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4900 robust_rms_before=0.898 arcsec robust_rms_before_corrected=0.240 arcsec robust_rms_after=0.243 arcsec worst_quadrant_rms_before=0.274 worst_quadrant_rms_after=0.277
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.274 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits N_match=4900 sigma_overall_arcsec=0.248 sigma_q1_arcsec=0.252 sigma_q2_arcsec=0.275 sigma_q3_arcsec=0.214 sigma_q4_arcsec=0.231 n_q1=1155 n_q2=1307 n_q3=1221 n_q4=1217 worst_quadrant_to_overall_ratio=1.111
The image catalog is written to wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits -region wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.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_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits to local_wcs_cache/
'wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits' -> 'local_wcs_cache/wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits'
Saving the final (post-refit) wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits to local_wcs_cache/
'wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits' -> 'local_wcs_cache/wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits'
Saving the final (post-refit) wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits to local_wcs_cache/
'wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits' -> 'local_wcs_cache/wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits'
Saving the final (post-refit) wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits to local_wcs_cache/
'wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits' -> 'local_wcs_cache/wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits sigma_overall=0.259 worst_q_ratio=1.300
ref2=Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits sigma_overall=0.263 worst_q_ratio=1.303
new1=fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits sigma_overall=0.266 worst_q_ratio=1.082
new2=fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits sigma_overall=0.248 worst_q_ratio=1.111
reference average sigma_overall=0.261 worst_q_ratio=1.3015
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115_astrometric_residuals.png (4894 matched stars from wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.23 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116_astrometric_residuals.png (4895 matched stars from wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.23 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454_astrometric_residuals.png (4903 matched stars from wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.23 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455_astrometric_residuals.png (4900 matched stars from wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.22 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits'
Saving fully-calibrated image wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits'
Preparing the HTML report for the field Eri-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 03:22:58.02 -01:24:57.7: 12.30 +/- 0.01 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 03:06:00.85 +02:01:09.3: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 03:45:16.82 -01:47:43.7: 12.13 +/- 0.01 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 03:27:00.06 -02:50:22.1: 12.28 +/- 0.01 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 03:31:02.22 -02:14:32.2: 11.84 +/- 0.01 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 03:45:16.82 -01:47:43.7: 12.09 +/- 0.01 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 03:06:00.85 +02:01:09.3: 15.82 +/- 99.00 upperlimit
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 03:31:02.22 -02:14:32.2: 11.87 +/- 0.01 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 03:22:58.02 -01:24:57.7: 12.37 +/- 0.01 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 03:27:00.06 -02:50:22.1: 12.29 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.11 +/- 0.01
Forced photometry reference-image weighted average: 12.29 +/- 0.01
Forced photometry reference-image weighted average: 12.33 +/- 0.01
Forced photometry filter REJECTED candidate at 03:45:16.82 -01:47:43.7: ref_mag=12.11 +/- 0.01 new_mean_mag=12.1355 delta=-0.02 (need > 0.90)
Forced photometry reference-image weighted average: 11.86 +/- 0.01
Forced photometry filter REJECTED candidate at 03:27:00.06 -02:50:22.1: ref_mag=12.29 +/- 0.01 new_mean_mag=12.2546 delta=0.03 (need > 0.90)
Forced photometry filter REJECTED candidate at 03:22:58.02 -01:24:57.7: ref_mag=12.33 +/- 0.01 new_mean_mag=12.2974 delta=0.03 (need > 0.90)
Forced photometry filter REJECTED candidate at 03:31:02.22 -02:14:32.2: ref_mag=11.86 +/- 0.01 new_mean_mag=12.0227 delta=-0.17 (need > 0.90)
Adding exclusion_list_local.txt__out20466.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 11s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20445_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455
The candidate 20445_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20454_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455
The candidate 20454_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20465_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455
The candidate 20465_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20466_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455
Preparing report for the candidate 20466_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20475_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455
The candidate 20475_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455 did not pass the final checks
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 14s
Prepared the HTML report for the field Eri-01-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
03:06:00.85 +02:01:09.3
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/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits
SExtractor catalog cache: saved Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits.cat to cache
SExtractor catalog cache: saved Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
Creating symlink local_wcs_cache/wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
Creating symlink local_wcs_cache/wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits
Creating symlink local_wcs_cache/wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits exists and is non-empty
wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits exists and is non-empty
wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits exists and is non-empty
wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits (1st reference image)
verification OK: wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
Image size: 941.5'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 03:25:43.554 -02:00:23.97 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits (1st new image)
verification OK: wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits
Image size: 941.0'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 03:25:49.030 -01:57:18.59 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 03:25:43.554 -02:00:23.97
Second-epoch image center 03:25:49.030 -01:57:18.59
Angular distance between the image centers 0.0563 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits (2nd new image)
verification OK: wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits
Image size: 941.0'x626.6' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 03:25:52.189 -01:57:58.26 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 03:25:43.554 -02:00:23.97
Second-epoch image center 03:25:52.189 -01:57:58.26
Angular distance between the image centers 0.0541 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 03:25:49.030 -01:57:18.59
Second-epoch second image center 03:25:52.189 -01:57:58.26
Angular distance between the image centers 0.01716 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/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits &> /tmp/tmp.qJsjruHlB3
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits &> /tmp/tmp.zRcCIwrK4N
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits &> /tmp/tmp.9b2FD4Sf38
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits &> /tmp/tmp.ZW9vJ0vUWe
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits
Calibrating the magnitude scale
Found non-empty wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.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_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits and wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.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_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits and wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits.wcscat
Found non-empty wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits and wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits.wcscat
The reference image (wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits) and catalog (wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits.wcscat) found
'wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits.wcscat' -> 'wcsmag.cat'
Read 38842 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 43.5260 to 59.3942 deg, Dec -7.3141 to +3.3249 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 43.5260 to 59.3942 deg, Dec -7.3141 to 3.3249 deg
Loaded 4661 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): 3618 out of 4007 total matches.
Matched with Tycho-2 4007 out of 38842 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.808100
a=0.000000 b=1.000000 c=22.808100
From vast_summary.log: estimated ref. image limiting mag.: -7.29
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.52
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.52
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 38842 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 43.5260 to 59.3942 deg, Dec -7.3141 to +3.3249 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 43.5260 to 59.3942 deg, Dec -7.3141 to 3.3249 deg
Loaded 4661 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): 3618 out of 4007 total matches.
Matched with Tycho-2 4007 out of 38842 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
Forced-photometry filter: calibrated wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits -> calib.txt_param_ref_wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits (aperture=4.8)
Read 38876 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 43.5102 to 59.3884 deg, Dec -7.3192 to +3.3177 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 43.5102 to 59.3884 deg, Dec -7.3192 to 3.3177 deg
Loaded 4658 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): 3627 out of 4001 total matches.
Matched with Tycho-2 4001 out of 38876 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
Forced-photometry filter: calibrated wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits -> calib.txt_param_ref_wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits (aperture=4.8)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 22 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.9 pix Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
1.9 pix Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
2.6 pix fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits
2.6 pix fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits
Limiting magnitude estimates:
15.5 mag. Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
15.5 mag. Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
15.3 mag. fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits
15.3 mag. fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits
All-image limiting magnitude estimate: 15.3 (SNR ) 14.5 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.qJsjruHlB3 (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_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits' -> 'wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.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/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
WCS_IMAGE_NAME=wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
WCS-calibrated image found: wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
Checking if the catalog wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits.wcscat corresponding to the image wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits alredy exist and is non-empty...
Catalog wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits.wcscat corresponding to the image wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits
WCS catalog name: wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.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=9, blended=1673, bad_region=4, passed=38833
Got 38833 stars (including 37092 good ones) from the SExtractor catalog wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits.wcscat
util/solve_plate_with_UCAC5 got 38833 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 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: 4901 matched stars entering correct_measured_positions(), 4901 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.22"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4901 matched stars entering correct_measured_positions(), 38833 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4903 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4901 matched stars entering correct_measured_positions(), 38833 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Accuracy estimation diagnostic: 4901 matched stars entering correct_measured_positions(), 38833 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Excluding outliers - 4901 stars left (next iteration limit 5391)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.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_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits N_match=4901 sigma_overall_arcsec=0.252 sigma_q1_arcsec=0.322 sigma_q2_arcsec=0.251 sigma_q3_arcsec=0.224 sigma_q4_arcsec=0.222 n_q1=1231 n_q2=1165 n_q3=1361 n_q4=1144 worst_quadrant_to_overall_ratio=1.275
The image catalog is written to wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits -region wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.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.zRcCIwrK4N (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_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits' -> 'wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.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/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
WCS_IMAGE_NAME=wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
WCS-calibrated image found: wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
Checking if the catalog wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits.wcscat corresponding to the image wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits alredy exist and is non-empty...
Catalog wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits.wcscat corresponding to the image wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits
WCS catalog name: wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.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=1668, bad_region=4, passed=38854
Got 38854 stars (including 37119 good ones) from the SExtractor catalog wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits.wcscat
util/solve_plate_with_UCAC5 got 38854 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
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: 4901 matched stars entering correct_measured_positions(), 4901 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.22"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4901 matched stars entering correct_measured_positions(), 38854 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 4903 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4901 matched stars entering correct_measured_positions(), 38854 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Accuracy estimation diagnostic: 4901 matched stars entering correct_measured_positions(), 38854 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Excluding outliers - 4901 stars left (next iteration limit 5391)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.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_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits N_match=4901 sigma_overall_arcsec=0.256 sigma_q1_arcsec=0.327 sigma_q2_arcsec=0.258 sigma_q3_arcsec=0.229 sigma_q4_arcsec=0.224 n_q1=1233 n_q2=1169 n_q3=1356 n_q4=1143 worst_quadrant_to_overall_ratio=1.280
The image catalog is written to wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits -region wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.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.9b2FD4Sf38 (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_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.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_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits
WCS_IMAGE_NAME=wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits
WCS-calibrated image found: wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits
Checking if the catalog wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits.wcscat corresponding to the image wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits alredy exist and is non-empty...
Catalog wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits.wcscat corresponding to the image wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits
WCS catalog name: wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.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=6, blended=1272, bad_region=21, passed=33759
Got 33759 stars (including 32426 good ones) from the SExtractor catalog wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits.wcscat
util/solve_plate_with_UCAC5 got 33759 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 412 to 470 (Dec -7.6 to 3.7)
Done reading UCAC5 zone files...
Matched 4900 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: 0.24"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4897 matched stars entering correct_measured_positions(), 33759 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 412 to 470 (Dec -7.6 to 3.7)
Done reading UCAC5 zone files...
Matched 4900 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4896 matched stars entering correct_measured_positions(), 33759 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.24"
Accuracy estimation diagnostic: 4896 matched stars entering correct_measured_positions(), 33759 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.25"
Excluding outliers - 4896 stars left (next iteration limit 5386)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.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=4896 robust_rms=10.216 arcsec worst_quadrant_rms=10.581 arcsec
SIP_REFIT: SIP order 3 trial: matched=4896 robust_rms=0.345 arcsec worst_quadrant_rms=0.356 arcsec
SIP_REFIT: SIP order 5 trial: matched=4896 robust_rms=0.247 arcsec worst_quadrant_rms=0.267 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4896 robust_rms_before=0.932 arcsec robust_rms_before_corrected=0.254 arcsec robust_rms_after=0.247 arcsec worst_quadrant_rms_before=0.274 worst_quadrant_rms_after=0.267
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.274 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits N_match=4896 sigma_overall_arcsec=0.266 sigma_q1_arcsec=0.269 sigma_q2_arcsec=0.286 sigma_q3_arcsec=0.241 sigma_q4_arcsec=0.246 n_q1=1150 n_q2=1287 n_q3=1237 n_q4=1222 worst_quadrant_to_overall_ratio=1.076
The image catalog is written to wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits -region wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.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.ZW9vJ0vUWe (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_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.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_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits
WCS_IMAGE_NAME=wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits
WCS-calibrated image found: wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits
Checking if the catalog wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits.wcscat corresponding to the image wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits alredy exist and is non-empty...
Catalog wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits.wcscat corresponding to the image wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits
WCS catalog name: wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.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=10, blended=1283, bad_region=29, passed=33469
Got 33469 stars (including 32104 good ones) from the SExtractor catalog wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits.wcscat
util/solve_plate_with_UCAC5 got 33469 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.0'
Seting catalog search parameters based on the expected field of view 941.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013069 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010456 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 412 to 470 (Dec -7.6 to 3.7)
Done reading UCAC5 zone files...
Matched 4901 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4898 matched stars entering correct_measured_positions(), 4898 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4898 matched stars entering correct_measured_positions(), 33469 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.22"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 412 to 470 (Dec -7.6 to 3.7)
Done reading UCAC5 zone files...
Matched 4901 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4899 matched stars entering correct_measured_positions(), 33469 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Accuracy estimation diagnostic: 4899 matched stars entering correct_measured_positions(), 33469 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.23"
Excluding outliers - 4899 stars left (next iteration limit 5387)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.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=4899 robust_rms=10.181 arcsec worst_quadrant_rms=10.505 arcsec
SIP_REFIT: SIP order 3 trial: matched=4899 robust_rms=0.315 arcsec worst_quadrant_rms=0.334 arcsec
SIP_REFIT: SIP order 5 trial: matched=4899 robust_rms=0.242 arcsec worst_quadrant_rms=0.277 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4899 robust_rms_before=0.896 arcsec robust_rms_before_corrected=0.243 arcsec robust_rms_after=0.242 arcsec worst_quadrant_rms_before=0.278 worst_quadrant_rms_after=0.277
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.278 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits N_match=4899 sigma_overall_arcsec=0.252 sigma_q1_arcsec=0.255 sigma_q2_arcsec=0.278 sigma_q3_arcsec=0.222 sigma_q4_arcsec=0.229 n_q1=1145 n_q2=1295 n_q3=1238 n_q4=1221 worst_quadrant_to_overall_ratio=1.104
The image catalog is written to wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits -region wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.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_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.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_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-53-34_20.00sec_-0.00C_LIGHTs_0454.fits
Saving fully-calibrated image wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.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_2026-09-12_CI_Eri-01-Q1b1x1_045520_TTUQ1b1x1_3903194_kC8jFMtX/wcs_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455.fits
Preparing the HTML report for the field Eri-01-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 03:36:20.92 -03:56:50.5: 14.97 +/- 0.14 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 03:36:16.34 -01:26:56.4: 14.16 +/- 0.06 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 03:14:32.99 +01:07:07.5: 13.48 +/- 0.04 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 03:08:39.81 +01:00:15.3: 14.78 +/- 0.13 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 03:02:35.68 +02:42:25.2: 14.73 +/- 0.12 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 03:08:39.81 +01:00:15.3: 14.73 +/- 0.12 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 02:58:10.41 -02:53:07.0: 13.63 +/- 0.05 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 03:36:20.92 -03:56:50.5: 15.01 +/- 0.14 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 03:02:35.68 +02:42:25.2: 14.89 +/- 0.15 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 03:14:53.33 +03:09:45.0: 15.99 +/- 99.00 upperlimit
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 03:14:32.99 +01:07:07.5: 13.39 +/- 0.03 detection
Forced photometry reference-image weighted average: 14.75 +/- 0.09
Forced photometry reference-image weighted average: 14.99 +/- 0.10
Forced photometry reference-image weighted average: 14.79 +/- 0.09
Forced photometry filter REJECTED candidate at 03:36:20.92 -03:56:50.5: ref_mag=14.99 +/- 0.10 new_mean_mag=14.7244 delta=0.26 (need > 0.90)
Forced photometry filter REJECTED candidate at 03:02:35.68 +02:42:25.2: ref_mag=14.79 +/- 0.09 new_mean_mag=14.7416 delta=0.05 (need > 0.90)
Forced photometry filter REJECTED candidate at 03:08:39.81 +01:00:15.3: ref_mag=14.75 +/- 0.09 new_mean_mag=14.4542 delta=0.30 (need > 0.90)
Forced photometry reference-image weighted average: 13.43 +/- 0.02
Forced photometry filter REJECTED candidate at 03:14:32.99 +01:07:07.5: ref_mag=13.43 +/- 0.02 new_mean_mag=13.6141 delta=-0.18 (need > 0.90)
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 03:36:16.34 -01:26:56.4: 14.10 +/- 0.06 detection
Forced photometry reference-image weighted average: 14.13 +/- 0.04
Forced photometry filter REJECTED candidate at 03:36:16.34 -01:26:56.4: ref_mag=14.13 +/- 0.04 new_mean_mag=14.2850 delta=-0.16 (need > 0.90)
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 03:18:53.54 -01:02:00.9: 14.44 +/- 0.08 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 03:04:33.19 -01:48:06.0: 14.96 +/- 0.14 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 03:14:53.33 +03:09:45.0: 16.00 +/- 99.00 upperlimit
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 02:58:10.41 -02:53:07.0: 13.62 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.62 +/- 0.03
Forced photometry filter REJECTED candidate at 02:58:10.41 -02:53:07.0: ref_mag=13.62 +/- 0.03 new_mean_mag=14.0347 delta=-0.41 (need > 0.90)
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 03:18:53.54 -01:02:00.9: 14.54 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.48 +/- 0.06
Forced photometry filter REJECTED candidate at 03:18:53.54 -01:02:00.9: ref_mag=14.48 +/- 0.06 new_mean_mag=14.4255 delta=0.05 (need > 0.90)
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 03:04:33.19 -01:48:06.0: 15.05 +/- 0.15 detection
Forced photometry reference-image weighted average: 15.00 +/- 0.10
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 03:05:25.99 +02:47:19.9: 15.02 +/- 0.16 detection
Forced photometry filter REJECTED candidate at 03:04:33.19 -01:48:06.0: ref_mag=15.00 +/- 0.10 new_mean_mag=14.7920 delta=0.21 (need > 0.90)
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 03:08:08.04 +02:40:04.5: 15.29 +/- 0.20 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 03:39:02.98 -02:54:57.6: 15.07 +/- 0.15 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 03:15:33.30 -02:11:20.8: 15.11 +/- 0.15 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 03:05:52.86 -01:52:25.2: 15.22 +/- 0.18 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 03:25:17.10 -01:09:46.1: 14.90 +/- 0.12 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 03:05:25.99 +02:47:19.9: 15.08 +/- 0.17 detection
Forced photometry reference-image weighted average: 15.05 +/- 0.12
Forced photometry filter REJECTED candidate at 03:05:25.99 +02:47:19.9: ref_mag=15.05 +/- 0.12 new_mean_mag=14.8919 delta=0.15 (need > 0.90)
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 03:09:54.72 -05:00:29.6: 15.08 +/- 0.15 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 03:39:02.98 -02:54:57.6: 15.00 +/- 0.14 detection
Forced photometry reference-image weighted average: 15.03 +/- 0.10
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 03:15:33.30 -02:11:20.8: 15.14 +/- 0.16 detection
Forced photometry filter REJECTED candidate at 03:39:02.98 -02:54:57.6: ref_mag=15.03 +/- 0.10 new_mean_mag=14.8345 delta=0.20 (need > 0.90)
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 03:08:08.04 +02:40:04.5: 15.34 +/- 0.21 detection
Forced photometry reference-image weighted average: 15.12 +/- 0.11
Forced photometry filter REJECTED candidate at 03:15:33.30 -02:11:20.8: ref_mag=15.12 +/- 0.11 new_mean_mag=14.8897 delta=0.23 (need > 0.90)
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 03:05:52.86 -01:52:25.2: 15.13 +/- 0.17 detection
Forced photometry reference-image weighted average: 15.31 +/- 0.15
Forced photometry filter REJECTED candidate at 03:08:08.04 +02:40:04.5: ref_mag=15.31 +/- 0.15 new_mean_mag=14.8524 delta=0.46 (need > 0.90)
Forced photometry reference-image weighted average: 15.17 +/- 0.12
Forced photometry filter REJECTED candidate at 03:05:52.86 -01:52:25.2: ref_mag=15.17 +/- 0.12 new_mean_mag=14.8921 delta=0.28 (need > 0.90)
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 03:25:17.10 -01:09:46.1: 15.30 +/- 0.19 detection
Forced photometry reference-image weighted average: 15.02 +/- 0.10
Forced photometry filter REJECTED candidate at 03:25:17.10 -01:09:46.1: ref_mag=15.02 +/- 0.10 new_mean_mag=14.9915 delta=0.03 (need > 0.90)
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-14_20.00sec_-15.00C_LIGHT_0115.fits at 03:53:59.62 +02:29:52.6: 15.16 +/- 0.21 detection
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 03:09:54.72 -05:00:29.6: 14.86 +/- 0.13 detection
Forced photometry reference-image weighted average: 14.96 +/- 0.10
Forced photometry filter REJECTED candidate at 03:09:54.72 -05:00:29.6: ref_mag=14.96 +/- 0.10 new_mean_mag=14.8862 delta=0.07 (need > 0.90)
Forced photometry on wcs_Eri-01-Q1b1x1_2026-01-08_21-44-53_20.00sec_-15.00C_LIGHT_0116.fits at 03:53:59.62 +02:29:52.6: 15.14 +/- 0.22 detection
Forced photometry reference-image weighted average: 15.15 +/- 0.15
Forced photometry filter REJECTED candidate at 03:53:59.62 +02:29:52.6: ref_mag=15.15 +/- 0.15 new_mean_mag=14.8516 delta=0.30 (need > 0.90)
Adding exclusion_list_local.txt__out53092.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 8s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 52659_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455
The candidate 52659_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455 did not pass the final checks
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Considering the candidate 52662_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455
The candidate 52662_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455 did not pass the final checks
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Considering the candidate 52672_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455
The candidate 52672_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455 did not pass the final checks
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Considering the candidate 52846_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455
The candidate 52846_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455 did not pass the final checks
**** FOUND 03:06:00.85 +02:01:09.3 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53092_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455
Preparing report for the candidate 53092_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455
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Considering the candidate 53145_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455
The candidate 53145_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455 did not pass the final checks
**** FOUND 03:32:20.54 -07:05:00.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53162_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455
The candidate 53162_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455 did not pass the final checks
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Considering the candidate 53279_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455
The candidate 53279_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455 did not pass the final checks
**** FOUND 03:27:09.25 -03:15:26.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53447_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455
The candidate 53447_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455 did not pass the final checks
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Considering the candidate 53470_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455
The candidate 53470_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455 did not pass the final checks
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Considering the candidate 53479_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455
The candidate 53479_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455 did not pass the final checks
**** FOUND 03:12:32.02 +01:56:19.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53525_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455
The candidate 53525_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455 did not pass the final checks
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Considering the candidate 53680_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455
The candidate 53680_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455 did not pass the final checks
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Considering the candidate 53718_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455
The candidate 53718_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455 did not pass the final checks
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Considering the candidate 53725_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455
The candidate 53725_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455 did not pass the final checks
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Considering the candidate 53750_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455
The candidate 53750_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455 did not pass the final checks
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Considering the candidate 53761_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455
The candidate 53761_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455 did not pass the final checks
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Considering the candidate 53780_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455
The candidate 53780_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455 did not pass the final checks
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Considering the candidate 53785_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455
The candidate 53785_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455 did not pass the final checks
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Considering the candidate 53802_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455
The candidate 53802_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455 did not pass the final checks
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Considering the candidate 53840_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455
The candidate 53840_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455 did not pass the final checks
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Considering the candidate 28839_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455
The candidate 28839_fd_Eri-01-Q1b1x1_2026-09-12_04-54-39_20.00sec_-0.00C_LIGHTs_0455 did not pass the final checks