This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461320.8713,8.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261007.3713 8.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461320.8713,8.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261007.3713 8.38CV 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 10 07.3713 2461320.8713 14.38 00:14:10.04 +00:27:24.3
103.42596 -60.99562 galactic Psc Second-epoch detections are separated by 1.7" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.1735 ITA -0 0 0 14.5 0 0
Forced photometry on wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 00:14:10.04 +00:27:24.3: 15.79 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 00:14:10.04 +00:27:24.3: 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!
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,2461320.8713,14.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20261007.3713 14.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461242.92203095 21.07.2026 10:07:33.474 /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
First image: 2461242.92203095 21.07.2026 10:07:33.474 /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
Last image: 2461320.87155890 07.10.2026 08:54:52.689 /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.37
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: 14 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): 5456
Objects passed selection criteria: 5437
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 4295.5
Average stars matched: 3882.75 (90.3911 %)
Memory usage VmPeak: 231552 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Oct 6 12:01:37 CDT 2026
VaST build number 1.0rc89-233-gd5bdb823
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-06)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Oct 7 10:13:33 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461242.92203095 21.07.2026 10:07:33.474 /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
First image: 2461242.92203095 21.07.2026 10:07:33.474 /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
Last image: 2461320.87155890 07.10.2026 08:54:52.689 /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 206
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.12
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: 78 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): 29320
Objects passed selection criteria: 29212
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 23792.2
Average stars matched: 21356.2 (89.7614 %)
Memory usage VmPeak: 250172 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Tue Oct 6 12:01:37 CDT 2026
VaST build number 1.0rc89-233-gd5bdb823
OpenMP enabled: Yes
SExtractor version 2.25.2 (2026-10-06)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Oct 7 10:16:27 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits
SExtractor catalog cache: saved Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits.cat to cache
SExtractor catalog cache: saved Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461320.87111082
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits exists and is non-empty
wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits exists and is non-empty
wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits exists and is non-empty
wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits (1st reference image)
verification OK: wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
Image size: 937.3'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:00:00.424 -02:00:17.62 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits (1st new image)
verification OK: wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits
Image size: 937.3'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:00:00.820 -01:59:51.91 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:00:00.424 -02:00:17.62
Second-epoch image center 00:00:00.820 -01:59:51.91
Angular distance between the image centers 0.0073 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits (2nd new image)
verification OK: wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits
Image size: 939.3'x626.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.89"/pix along the X axis and 5.88"/pix along the Y axis
Image center: 23:59:59.724 -01:59:41.20 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:00:00.424 -02:00:17.62
Second-epoch image center 23:59:59.724 -01:59:41.20
Angular distance between the image centers 0.0105 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 00:00:00.820 -01:59:51.91
Second-epoch second image center 23:59:59.724 -01:59:41.20
Angular distance between the image centers 0.00545 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits &> /tmp/tmp.S4VHywqOIT
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits &> /tmp/tmp.WNX66RYnzU
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits &> /tmp/tmp.ucHYwisrLt
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits &> /tmp/tmp.rsHieWdFSW
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits and wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits and wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits.wcscat
Found non-empty wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits and wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits.wcscat
The reference image (wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits) and catalog (wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits.wcscat) found
'wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits.wcscat' -> 'wcsmag.cat'
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 5537 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 352.1391 to 7.8851 deg, Dec -7.2685 to +3.2742 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 352.1391 to 7.8851 deg, Dec -7.2685 to 3.2742 deg
Loaded 113496 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): 3358 out of 3443 total matches.
Matched with Tycho-2 3443 out of 5537 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.632850
a=0.000000 b=1.000000 c=22.632850
From vast_summary.log: estimated ref. image limiting mag.: -7.37
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.26
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.26
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 5537 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 352.1391 to 7.8851 deg, Dec -7.2685 to +3.2742 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 352.1391 to 7.8851 deg, Dec -7.2685 to 3.2742 deg
Loaded 113496 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): 3358 out of 3443 total matches.
Matched with Tycho-2 3443 out of 5537 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
Forced-photometry filter: calibrated wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits -> calib.txt_param_ref_wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits (aperture=6.3)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 5464 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 352.1355 to 7.8705 deg, Dec -7.2684 to +3.2771 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 352.1355 to 7.8705 deg, Dec -7.2684 to 3.2771 deg
Loaded 113493 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): 3322 out of 3420 total matches.
Matched with Tycho-2 3420 out of 5464 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits
Forced-photometry filter: calibrated wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits -> calib.txt_param_ref_wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits (aperture=6.3)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.3 pix Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
2.2 pix Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits
2.3 pix fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits
2.3 pix fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits
Limiting magnitude estimates:
15.3 mag. Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
15.3 mag. Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits
15.3 mag. fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits
15.3 mag. fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits
All-image limiting magnitude estimate: 15.3 (SNR ) 12.0 (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.S4VHywqOIT (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_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits' -> 'wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
WCS_IMAGE_NAME=wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
WCS-calibrated image found: wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
Checking if the catalog wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits.wcscat corresponding to the image wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits alredy exist and is non-empty...
Catalog wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits.wcscat corresponding to the image wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
WCS catalog name: wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=342, bad_region=1203, passed=5537
Got 5537 stars (including 4070 good ones) from the SExtractor catalog wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits.wcscat
util/solve_plate_with_UCAC5 got 5537 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 352.1391 through 0 to 7.8851, gap 7.8851 to 352.1391
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 3977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3972 matched stars entering correct_measured_positions(), 3972 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3972 matched stars entering correct_measured_positions(), 4582 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 352.1393 through 0 to 7.8851, gap 7.8851 to 352.1393
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 3977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3972 matched stars entering correct_measured_positions(), 4582 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 3972 matched stars entering correct_measured_positions(), 4582 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 3972 stars left (next iteration limit 4369)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits N_match=3972 sigma_overall_arcsec=0.303 sigma_q1_arcsec=0.272 sigma_q2_arcsec=0.295 sigma_q3_arcsec=0.350 sigma_q4_arcsec=0.283 n_q1=1263 n_q2=686 n_q3=1324 n_q4=699 worst_quadrant_to_overall_ratio=1.153
The image catalog is written to wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits -region wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.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.WNX66RYnzU (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_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits' -> 'wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits
WCS_IMAGE_NAME=wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits
WCS-calibrated image found: wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits
Checking if the catalog wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits.wcscat corresponding to the image wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits alredy exist and is non-empty...
Catalog wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits.wcscat corresponding to the image wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits
WCS catalog name: wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=3, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=354, bad_region=1178, passed=5461
Got 5461 stars (including 4010 good ones) from the SExtractor catalog wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits.wcscat
util/solve_plate_with_UCAC5 got 5461 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 352.1355 through 0 to 7.8705, gap 7.8705 to 352.1355
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 3920 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3914 matched stars entering correct_measured_positions(), 3914 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3914 matched stars entering correct_measured_positions(), 4515 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 352.1357 through 0 to 7.8705, gap 7.8705 to 352.1357
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 3920 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3913 matched stars entering correct_measured_positions(), 4515 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 3913 matched stars entering correct_measured_positions(), 4515 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 3913 stars left (next iteration limit 4305)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits N_match=3913 sigma_overall_arcsec=0.351 sigma_q1_arcsec=0.311 sigma_q2_arcsec=0.347 sigma_q3_arcsec=0.401 sigma_q4_arcsec=0.331 n_q1=1258 n_q2=678 n_q3=1296 n_q4=681 worst_quadrant_to_overall_ratio=1.142
The image catalog is written to wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits -region wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.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.ucHYwisrLt (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_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.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_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits
WCS_IMAGE_NAME=wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits
WCS-calibrated image found: wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits
Checking if the catalog wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits.wcscat corresponding to the image wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits.wcscat corresponding to the image wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits
WCS catalog name: wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=306, bad_region=1261, passed=5600
Got 5600 stars (including 4081 good ones) from the SExtractor catalog wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits.wcscat
util/solve_plate_with_UCAC5 got 5600 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 352.1558 through 0 to 7.8986, gap 7.8986 to 352.1558
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 3988 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3982 matched stars entering correct_measured_positions(), 3982 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3982 matched stars entering correct_measured_positions(), 4590 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 352.1560 through 0 to 7.8991, gap 7.8991 to 352.1560
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 3988 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3982 matched stars entering correct_measured_positions(), 4590 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 3982 matched stars entering correct_measured_positions(), 4590 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 3982 stars left (next iteration limit 4380)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=3982 robust_rms=7.644 arcsec worst_region_rms=13.831 arcsec outer_annulus_rms=13.831 arcsec
SIP_REFIT: SIP order 3 trial: matched=3982 robust_rms=0.478 arcsec worst_region_rms=0.836 arcsec outer_annulus_rms=0.836 arcsec
SIP_REFIT: SIP order 5 trial: matched=3982 robust_rms=0.329 arcsec worst_region_rms=0.368 arcsec outer_annulus_rms=0.368 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3982 robust_rms_before=0.900 arcsec robust_rms_before_corrected=0.311 arcsec robust_rms_after=0.329 arcsec worst_region_rms_before=0.369 worst_region_rms_after=0.368 outer_annulus_rms_before=1.205 outer_annulus_rms_after=0.368
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.369 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits worst_region_rms_kept=0.369 arcsec robust_rms_kept=0.311 arcsec matched=3982
WCS_QUALITY_DIAG: file=fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits N_match=3982 sigma_overall_arcsec=0.321 sigma_q1_arcsec=0.320 sigma_q2_arcsec=0.330 sigma_q3_arcsec=0.319 sigma_q4_arcsec=0.319 n_q1=1246 n_q2=805 n_q3=1196 n_q4=735 worst_quadrant_to_overall_ratio=1.028
The image catalog is written to wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits -region wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.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.rsHieWdFSW (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_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.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_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits
WCS_IMAGE_NAME=wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits
WCS-calibrated image found: wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits
Checking if the catalog wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits.wcscat corresponding to the image wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits.wcscat corresponding to the image wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits
WCS catalog name: wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=310, bad_region=1272, passed=5609
Got 5609 stars (including 4076 good ones) from the SExtractor catalog wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits.wcscat
util/solve_plate_with_UCAC5 got 5609 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.3'
Seting catalog search parameters based on the expected field of view 939.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013046 (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 0.010437 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 352.1322 through 0 to 7.8938, gap 7.8938 to 352.1322
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 3932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3849 matched stars entering correct_measured_positions(), 3849 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.96"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 3815 matched stars entering correct_measured_positions(), 4563 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.97"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 352.1289 through 0 to 7.8877, gap 7.8877 to 352.1289
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 3978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 3964 matched stars entering correct_measured_positions(), 4570 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 3964 matched stars entering correct_measured_positions(), 4590 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 3964 stars left (next iteration limit 4196)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=3964 robust_rms=7.602 arcsec worst_region_rms=13.909 arcsec outer_annulus_rms=13.909 arcsec
SIP_REFIT: SIP order 3 trial: matched=3964 robust_rms=0.432 arcsec worst_region_rms=0.638 arcsec outer_annulus_rms=0.638 arcsec
SIP_REFIT: SIP order 5 trial: matched=3964 robust_rms=0.322 arcsec worst_region_rms=0.359 arcsec outer_annulus_rms=0.351 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3964 robust_rms_before=13.839 arcsec robust_rms_before_corrected=1.064 arcsec robust_rms_after=0.322 arcsec worst_region_rms_before=3.074 worst_region_rms_after=0.359 outer_annulus_rms_before=31.163 outer_annulus_rms_after=0.351
verification OK: wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits
verification OK: wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits
Image size: 937.5'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:59:59.740 -01:59:37.84 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 5609 stars ###
'wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/correct_sextractor_wcs_catalog_usingxy2sky3123741.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 13.839 -> 0.322 arcsec)
SIP_REFIT: re-matching the catalog with the refit solution (cycle 1, search radius 3.0 arcsec, 3964 pairs from the previous matching)
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 352.1388 through 0 to 7.8852, gap 7.8852 to 352.1388
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 3835 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
SIP_REFIT: re-match found 3835 pairs (3964 from the previous matching)
SIP_REFIT: SIP order 2 trial: matched=3835 robust_rms=7.642 arcsec worst_region_rms=14.847 arcsec outer_annulus_rms=14.847 arcsec
SIP_REFIT: SIP order 3 trial: matched=3835 robust_rms=0.431 arcsec worst_region_rms=0.643 arcsec outer_annulus_rms=0.643 arcsec
SIP_REFIT: SIP order 5 trial: matched=3835 robust_rms=0.322 arcsec worst_region_rms=0.359 arcsec outer_annulus_rms=0.359 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=3835 robust_rms_before=0.321 arcsec robust_rms_before_corrected=0.321 arcsec robust_rms_after=0.322 arcsec worst_region_rms_before=0.361 worst_region_rms_after=0.359 outer_annulus_rms_before=0.361 outer_annulus_rms_after=0.359
verification OK: wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits
verification OK: wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits
Image size: 937.5'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:59:59.740 -01:59:37.83 J2000 4789.000 3195.000
### Converting SExtractor-derived pixel positions to celestial coordinates using xy2sky from WCSTools ###
### Converted positions of 5609 stars ###
'wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits.wcscat' -> 'vast_debug_catalog_before_xy2sky_correction.cat.log'
'/data_ssd/NMW-TexasTech/workdir/vast_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/correct_sextractor_wcs_catalog_usingxy2sky3124909.tmp' -> 'vast_debug_catalog_after_xy2sky_correction.cat.log'
SIP_REFIT: applied the refit solution (order 5, robust RMS 0.321 -> 0.322 arcsec)
Accuracy estimation diagnostic: 3835 matched stars entering correct_measured_positions(), 4590 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 3835 matched stars entering correct_measured_positions(), 4587 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
WCS_QUALITY_DIAG: file=fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits N_match=3835 sigma_overall_arcsec=0.341 sigma_q1_arcsec=0.332 sigma_q2_arcsec=0.338 sigma_q3_arcsec=0.330 sigma_q4_arcsec=0.379 n_q1=1232 n_q2=769 n_q3=1121 n_q4=713 worst_quadrant_to_overall_ratio=1.113
The image catalog is written to wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits -region wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits to local_wcs_cache/
'wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits' -> 'local_wcs_cache/wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits'
Saving the final (post-refit) wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits to local_wcs_cache/
'wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits' -> 'local_wcs_cache/wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits'
Saving the final (post-refit) wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits to local_wcs_cache/
'wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits' -> 'local_wcs_cache/wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits'
Saving the final (post-refit) wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits to local_wcs_cache/
'wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits' -> 'local_wcs_cache/wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits sigma_overall=0.303 worst_q_ratio=1.153
ref2=Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits sigma_overall=0.351 worst_q_ratio=1.142
new1=fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits sigma_overall=0.321 worst_q_ratio=1.028
new2=fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits sigma_overall=0.341 worst_q_ratio=1.113
reference average sigma_overall=0.327 worst_q_ratio=1.1475
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999_astrometric_residuals.png (3972 matched stars from wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.27 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000_astrometric_residuals.png (3913 matched stars from wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.30 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390_astrometric_residuals.png (3982 matched stars from wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.29 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391_astrometric_residuals.png (3835 matched stars from wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.24 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits'
Saving fully-calibrated image wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits'
Preparing the HTML report for the field Psc-08-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 23:58:44.46 -01:12:34.2: 12.06 +/- 0.01 detection
Forced photometry on wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 23:54:14.08 +02:14:52.1: 11.83 +/- 0.01 detection
Forced photometry on wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 23:58:44.46 -01:12:34.2: 12.04 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.05 +/- 0.01
Forced photometry on wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 23:54:14.08 +02:14:52.1: 11.80 +/- 0.01 detection
Forced photometry filter REJECTED candidate at 23:58:44.46 -01:12:34.2: ref_mag=12.05 +/- 0.01 new_mean_mag=12.0270 delta=0.02 (need > 0.90)
Forced photometry reference-image weighted average: 11.82 +/- 0.01
Forced photometry filter REJECTED candidate at 23:54:14.08 +02:14:52.1: ref_mag=11.82 +/- 0.01 new_mean_mag=12.0420 delta=-0.23 (need > 0.90)
make_report_in_HTML.sh Phase 1 (network queries): 7s
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: 4s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20254_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
Preparing report for the candidate 20254_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21042_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 21042_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21047_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 21047_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 11s
Prepared the HTML report for the field Psc-08-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits
SExtractor catalog cache: saved Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits.cat to cache
SExtractor catalog cache: saved Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
Creating symlink local_wcs_cache/wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits
Creating symlink local_wcs_cache/wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits exists and is non-empty
wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits exists and is non-empty
wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits exists and is non-empty
wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits (1st reference image)
verification OK: wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
Image size: 937.3'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:00:00.424 -02:00:17.62 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits (1st new image)
verification OK: wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits
Image size: 937.3'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 00:00:00.820 -01:59:51.91 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 00:00:00.424 -02:00:17.62
Second-epoch image center 00:00:00.820 -01:59:51.91
Angular distance between the image centers 0.0073 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits (2nd new image)
verification OK: wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits
Image size: 937.5'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 23:59:59.740 -01:59:37.83 J2000 4789.000 3195.000
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# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 00:00:00.424 -02:00:17.62
Second-epoch image center 23:59:59.740 -01:59:37.83
Angular distance between the image centers 0.0114 deg.
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# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 00:00:00.820 -01:59:51.91
Second-epoch second image center 23:59:59.740 -01:59:37.83
Angular distance between the image centers 0.00596 deg.
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Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits &> /tmp/tmp.weq8hwp35P
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits &> /tmp/tmp.nSipIgKkfA
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits &> /tmp/tmp.Z1vMQ1Pwj9
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits &> /tmp/tmp.gb30ZvHd8f
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits
Calibrating the magnitude scale
Found non-empty wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits and wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits.wcscat
wait (drain background util/solve_plate_with_UCAC5 jobs before Tycho-2 calibration -- avoids wcs_.fits write race)
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits and wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits.wcscat
Found non-empty wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits and wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits.wcscat
The reference image (wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits) and catalog (wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits.wcscat) found
'wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits.wcscat' -> 'wcsmag.cat'
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 29281 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 352.1384 to 7.8963 deg, Dec -7.2757 to +3.2741 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 352.1384 to 7.8963 deg, Dec -7.2757 to 3.2741 deg
Loaded 113505 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): 3329 out of 3554 total matches.
Matched with Tycho-2 3554 out of 29281 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.525300
a=0.000000 b=1.000000 c=22.525300
From vast_summary.log: estimated ref. image limiting mag.: -7.12
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.41
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.41
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 29281 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 352.1384 to 7.8963 deg, Dec -7.2757 to +3.2741 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 352.1384 to 7.8963 deg, Dec -7.2757 to 3.2741 deg
Loaded 113505 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): 3329 out of 3554 total matches.
Matched with Tycho-2 3554 out of 29281 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
Forced-photometry filter: calibrated wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits -> calib.txt_param_ref_wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits (aperture=5.0)
The field straddles RA=0: the RA boundaries wrap around (min > max)
Read 30046 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 352.1258 to 7.8769 deg, Dec -7.2751 to +3.2772 deg
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Tycho-2 catalog search boundaries: RA 352.1258 to 7.8769 deg, Dec -7.2751 to 3.2772 deg
Loaded 113502 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): 3314 out of 3546 total matches.
Matched with Tycho-2 3546 out of 30046 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits
Forced-photometry filter: calibrated wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits -> calib.txt_param_ref_wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits (aperture=4.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 134 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.2 pix Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
2.1 pix Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits
2.2 pix fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits
2.2 pix fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits
Limiting magnitude estimates:
15.4 mag. Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
15.4 mag. Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits
15.4 mag. fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits
15.4 mag. fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits
All-image limiting magnitude estimate: 15.4 (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.weq8hwp35P (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_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits' -> 'wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
WCS_IMAGE_NAME=wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
WCS-calibrated image found: wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
Checking if the catalog wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits.wcscat corresponding to the image wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits alredy exist and is non-empty...
Catalog wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits.wcscat corresponding to the image wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits
WCS catalog name: wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=1084, bad_region=5467, passed=29269
Got 29269 stars (including 22908 good ones) from the SExtractor catalog wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits.wcscat
util/solve_plate_with_UCAC5 got 29269 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 352.1384 through 0 to 7.8963, gap 7.8963 to 352.1384
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 4857 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4850 matched stars entering correct_measured_positions(), 4850 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4850 matched stars entering correct_measured_positions(), 25114 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 352.1387 through 0 to 7.8963, gap 7.8963 to 352.1387
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 4857 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4850 matched stars entering correct_measured_positions(), 25114 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 4850 matched stars entering correct_measured_positions(), 25114 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 4850 stars left (next iteration limit 5335)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits N_match=4850 sigma_overall_arcsec=0.314 sigma_q1_arcsec=0.280 sigma_q2_arcsec=0.301 sigma_q3_arcsec=0.357 sigma_q4_arcsec=0.302 n_q1=1560 n_q2=873 n_q3=1533 n_q4=884 worst_quadrant_to_overall_ratio=1.137
The image catalog is written to wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits -region wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.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.nSipIgKkfA (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_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits' -> 'wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits
WCS_IMAGE_NAME=wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits
WCS-calibrated image found: wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits
Checking if the catalog wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits.wcscat corresponding to the image wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits alredy exist and is non-empty...
Catalog wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits.wcscat corresponding to the image wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits
WCS catalog name: wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=1265, bad_region=5561, passed=30034
Got 30034 stars (including 23398 good ones) from the SExtractor catalog wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits.wcscat
util/solve_plate_with_UCAC5 got 30034 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 352.1258 through 0 to 7.8769, gap 7.8769 to 352.1258
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 4861 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4854 matched stars entering correct_measured_positions(), 4854 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4854 matched stars entering correct_measured_positions(), 25818 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 352.1262 through 0 to 7.8769, gap 7.8769 to 352.1262
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 4861 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4854 matched stars entering correct_measured_positions(), 25818 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4854 matched stars entering correct_measured_positions(), 25818 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 4854 stars left (next iteration limit 5339)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits N_match=4854 sigma_overall_arcsec=0.350 sigma_q1_arcsec=0.313 sigma_q2_arcsec=0.350 sigma_q3_arcsec=0.404 sigma_q4_arcsec=0.340 n_q1=1568 n_q2=872 n_q3=1544 n_q4=870 worst_quadrant_to_overall_ratio=1.153
The image catalog is written to wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits -region wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.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.Z1vMQ1Pwj9 (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_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.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_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits
WCS_IMAGE_NAME=wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits
WCS-calibrated image found: wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits
Checking if the catalog wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits.wcscat corresponding to the image wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits.wcscat corresponding to the image wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits
WCS catalog name: wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=1149, bad_region=4749, passed=28524
Got 28524 stars (including 22937 good ones) from the SExtractor catalog wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits.wcscat
util/solve_plate_with_UCAC5 got 28524 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 352.1449 through 0 to 7.9091, gap 7.9091 to 352.1449
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 4838 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4829 matched stars entering correct_measured_positions(), 4829 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4829 matched stars entering correct_measured_positions(), 24974 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 352.1451 through 0 to 7.9098, gap 7.9098 to 352.1451
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 4838 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4829 matched stars entering correct_measured_positions(), 24974 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4829 matched stars entering correct_measured_positions(), 24975 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4829 stars left (next iteration limit 5311)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.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=4829 robust_rms=7.458 arcsec worst_region_rms=13.847 arcsec outer_annulus_rms=13.847 arcsec
SIP_REFIT: SIP order 3 trial: matched=4829 robust_rms=0.480 arcsec worst_region_rms=0.811 arcsec outer_annulus_rms=0.811 arcsec
SIP_REFIT: SIP order 5 trial: matched=4829 robust_rms=0.335 arcsec worst_region_rms=0.371 arcsec outer_annulus_rms=0.371 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4829 robust_rms_before=0.907 arcsec robust_rms_before_corrected=0.312 arcsec robust_rms_after=0.335 arcsec worst_region_rms_before=0.381 worst_region_rms_after=0.371 outer_annulus_rms_before=1.162 outer_annulus_rms_after=0.371
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.381 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits worst_region_rms_kept=0.381 arcsec robust_rms_kept=0.312 arcsec matched=4829
WCS_QUALITY_DIAG: file=fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits N_match=4829 sigma_overall_arcsec=0.325 sigma_q1_arcsec=0.315 sigma_q2_arcsec=0.332 sigma_q3_arcsec=0.317 sigma_q4_arcsec=0.326 n_q1=1540 n_q2=944 n_q3=1479 n_q4=866 worst_quadrant_to_overall_ratio=1.021
The image catalog is written to wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits -region wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.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.gb30ZvHd8f (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_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.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_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits
WCS_IMAGE_NAME=wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits
WCS-calibrated image found: wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits
Checking if the catalog wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits.wcscat corresponding to the image wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits alredy exist and is non-empty...
Catalog wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits.wcscat corresponding to the image wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits
WCS catalog name: wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits.wcscat
Excluding image region: -1.0 -1.0 1.0 1.0 (defined in bad_region.lst)
Excluding image region: 7500.0 0.0 9576.0 6388.0 (defined in bad_region.lst)
Excluding image region: 1122.0 1550.0 1124.0 1552.0 (defined in bad_region.lst)
Excluding image region: 1637.0 2824.0 1639.0 2826.0 (defined in bad_region.lst)
Excluding image region: 1831.0 2839.0 1833.0 2841.0 (defined in bad_region.lst)
Excluding image region: 1905.0 4570.0 1907.0 4572.0 (defined in bad_region.lst)
Excluding image region: 2012.0 4693.0 2014.0 4695.0 (defined in bad_region.lst)
Excluding image region: 2397.0 4241.0 2399.0 4243.0 (defined in bad_region.lst)
Excluding image region: 2679.0 2807.0 2681.0 2809.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 31 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=1176, bad_region=4764, passed=28572
Got 28572 stars (including 22942 good ones) from the SExtractor catalog wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits.wcscat
util/solve_plate_with_UCAC5 got 28572 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 352.1388 through 0 to 7.8969, gap 7.8969 to 352.1388
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 4835 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4825 matched stars entering correct_measured_positions(), 4825 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4825 matched stars entering correct_measured_positions(), 25003 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
RA wraps around 0/360 boundary: field RA 352.1388 through 0 to 7.8969, gap 7.8969 to 352.1388
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 4835 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4825 matched stars entering correct_measured_positions(), 25003 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 4825 matched stars entering correct_measured_positions(), 25003 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 4825 stars left (next iteration limit 5307)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.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=4825 robust_rms=7.475 arcsec worst_region_rms=14.010 arcsec outer_annulus_rms=14.010 arcsec
SIP_REFIT: SIP order 3 trial: matched=4825 robust_rms=0.437 arcsec worst_region_rms=0.678 arcsec outer_annulus_rms=0.678 arcsec
SIP_REFIT: SIP order 5 trial: matched=4825 robust_rms=0.331 arcsec worst_region_rms=0.379 arcsec outer_annulus_rms=0.379 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4825 robust_rms_before=0.331 arcsec robust_rms_before_corrected=0.306 arcsec robust_rms_after=0.331 arcsec worst_region_rms_before=0.378 worst_region_rms_after=0.379 outer_annulus_rms_before=0.378 outer_annulus_rms_after=0.379
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-region baseline 0.378 arcsec) - keeping the original
SIP_REFIT_REJECTED: file=fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits worst_region_rms_kept=0.378 arcsec robust_rms_kept=0.306 arcsec matched=4825
WCS_QUALITY_DIAG: file=fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits N_match=4825 sigma_overall_arcsec=0.313 sigma_q1_arcsec=0.299 sigma_q2_arcsec=0.316 sigma_q3_arcsec=0.316 sigma_q4_arcsec=0.330 n_q1=1529 n_q2=945 n_q3=1485 n_q4=866 worst_quadrant_to_overall_ratio=1.052
The image catalog is written to wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits -region wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Skipping WCS quality comparison: not the first SExtractor pass (default.sex.telephoto_lens_vSTL)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.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_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-13_20.00sec_-0.00C_LIGHT_0390.fits
Saving fully-calibrated image wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.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_2026-10-07_CI_Psc-08-Q2b1x1_100408_TTUQ2b1x1_2205319_gvidgJuN/wcs_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391.fits
Preparing the HTML report for the field Psc-08-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 23:57:47.33 +01:16:22.2: 14.56 +/- 0.12 detection
Forced photometry on wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 23:54:13.83 -00:07:51.2: 14.28 +/- 0.09 detection
Forced photometry on wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 00:16:01.56 -05:25:02.8: 14.06 +/- 0.08 detection
Forced photometry on wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 23:59:31.60 -00:03:35.2: 14.64 +/- 0.13 detection
Forced photometry on wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 23:54:52.12 +00:04:17.8: 12.70 +/- 0.03 detection
Forced photometry on wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 23:49:56.10 +01:54:09.2: 12.72 +/- 0.02 detection
Forced photometry on wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 23:54:13.83 -00:07:51.2: 14.28 +/- 0.09 detection
Forced photometry on wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 23:54:52.12 +00:04:17.8: 12.71 +/- 0.03 detection
Forced photometry reference-image weighted average: 14.28 +/- 0.06
Forced photometry filter REJECTED candidate at 23:54:13.83 -00:07:51.2: ref_mag=14.28 +/- 0.06 new_mean_mag=14.4705 delta=-0.19 (need > 0.90)
Forced photometry reference-image weighted average: 12.71 +/- 0.02
Forced photometry filter REJECTED candidate at 23:54:52.12 +00:04:17.8: ref_mag=12.71 +/- 0.02 new_mean_mag=12.7307 delta=-0.02 (need > 0.90)
Forced photometry on wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 23:57:47.33 +01:16:22.2: 14.50 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.53 +/- 0.08
Forced photometry filter REJECTED candidate at 23:57:47.33 +01:16:22.2: ref_mag=14.53 +/- 0.08 new_mean_mag=14.5257 delta=0.00 (need > 0.90)
Forced photometry on wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 00:16:01.56 -05:25:02.8: 14.05 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.06 +/- 0.05
Forced photometry on wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 23:59:31.60 -00:03:35.2: 14.52 +/- 0.11 detection
Forced photometry filter REJECTED candidate at 00:16:01.56 -05:25:02.8: ref_mag=14.06 +/- 0.05 new_mean_mag=13.9182 delta=0.14 (need > 0.90)
Forced photometry reference-image weighted average: 14.57 +/- 0.08
Forced photometry filter REJECTED candidate at 23:59:31.60 -00:03:35.2: ref_mag=14.57 +/- 0.08 new_mean_mag=14.5803 delta=-0.01 (need > 0.90)
Forced photometry on wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 23:49:56.10 +01:54:09.2: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.74 +/- 0.02
Forced photometry filter REJECTED candidate at 23:49:56.10 +01:54:09.2: ref_mag=12.74 +/- 0.02 new_mean_mag=13.0485 delta=-0.31 (need > 0.90)
Forced photometry on wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 23:47:44.02 +02:02:27.2: 13.25 +/- 0.04 detection
Forced photometry on wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 23:56:27.64 -00:35:54.3: 13.39 +/- 0.04 detection
Forced photometry on wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 23:47:44.02 +02:02:27.2: 13.30 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.27 +/- 0.03
Forced photometry filter REJECTED candidate at 23:47:44.02 +02:02:27.2: ref_mag=13.27 +/- 0.03 new_mean_mag=13.4306 delta=-0.16 (need > 0.90)
Forced photometry on wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 23:56:27.64 -00:35:54.3: 13.47 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.43 +/- 0.03
Forced photometry filter REJECTED candidate at 23:56:27.64 -00:35:54.3: ref_mag=13.43 +/- 0.03 new_mean_mag=13.6549 delta=-0.22 (need > 0.90)
Forced photometry on wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 23:55:27.90 +01:40:47.8: 14.43 +/- 0.11 detection
Forced photometry on wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 00:00:36.91 +00:12:02.1: 14.21 +/- 0.11 detection
Forced photometry on wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 23:55:27.90 +01:40:47.8: 14.54 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.47 +/- 0.09
Forced photometry filter REJECTED candidate at 23:55:27.90 +01:40:47.8: ref_mag=14.47 +/- 0.09 new_mean_mag=14.3558 delta=0.12 (need > 0.90)
Forced photometry on wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 00:14:10.04 +00:27:24.3: 15.79 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 00:00:36.91 +00:12:02.1: 13.99 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.08 +/- 0.07
Forced photometry filter REJECTED candidate at 00:00:36.91 +00:12:02.1: ref_mag=14.08 +/- 0.07 new_mean_mag=14.2973 delta=-0.22 (need > 0.90)
Forced photometry on wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 00:14:10.04 +00:27:24.3: 15.82 +/- 99.00 upperlimit
Forced photometry on wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 00:15:39.59 -06:10:40.2: 14.81 +/- 0.17 detection
Forced photometry on wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 00:15:39.59 -06:10:40.2: 14.75 +/- 0.15 detection
Forced photometry on wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 23:56:16.58 +01:44:36.1: 15.07 +/- 0.18 detection
Forced photometry reference-image weighted average: 14.78 +/- 0.11
Forced photometry filter REJECTED candidate at 00:15:39.59 -06:10:40.2: ref_mag=14.78 +/- 0.11 new_mean_mag=14.6201 delta=0.16 (need > 0.90)
Forced photometry on wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 23:46:39.22 -03:07:55.0: 14.30 +/- 0.10 detection
Forced photometry on wcs_Psc-08-Q2b1x1_2026-07-21_05-07-33_20.00sec_5.00C_LIGHT_0999.fits at 00:12:29.80 -05:23:44.5: 15.42 +/- 0.26 detection
Forced photometry on wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 23:56:16.58 +01:44:36.1: 14.83 +/- 0.15 detection
Forced photometry reference-image weighted average: 14.93 +/- 0.11
Forced photometry filter REJECTED candidate at 23:56:16.58 +01:44:36.1: ref_mag=14.93 +/- 0.11 new_mean_mag=14.6956 delta=0.23 (need > 0.90)
Forced photometry on wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 00:12:29.80 -05:23:44.5: 15.30 +/- 0.24 detection
Forced photometry reference-image weighted average: 15.35 +/- 0.18
Forced photometry filter REJECTED candidate at 00:12:29.80 -05:23:44.5: ref_mag=15.35 +/- 0.18 new_mean_mag=14.7974 delta=0.56 (need > 0.90)
Forced photometry on wcs_Psc-08-Q2b1x1_2026-07-21_05-08-38_20.00sec_5.00C_LIGHT_1000.fits at 23:46:39.22 -03:07:55.0: 14.37 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.33 +/- 0.07
Forced photometry filter REJECTED candidate at 23:46:39.22 -03:07:55.0: ref_mag=14.33 +/- 0.07 new_mean_mag=14.6286 delta=-0.30 (need > 0.90)
Adding exclusion_list_local.txt__out36443.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 17s
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: 4s
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Considering the candidate 32294_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 32294_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (21.4") between the two second-epoch detections
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Considering the candidate 32295_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 32295_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
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Considering the candidate 32296_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 32296_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
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Considering the candidate 32297_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 32297_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 32298_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 32298_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
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Considering the candidate 32299_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 32299_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
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Considering the candidate 32332_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
Preparing report for the candidate 32332_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
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Considering the candidate 32584_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 32584_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 32678_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 32678_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.3") between the two second-epoch detections
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Considering the candidate 32686_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 32686_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 33331_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 33331_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 33539_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 33539_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.3") between the two second-epoch detections
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Considering the candidate 33565_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 33565_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.6") between the two second-epoch detections
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Considering the candidate 33656_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 33656_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.1") between the two second-epoch detections
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Considering the candidate 33711_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 33711_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
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Considering the candidate 33716_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 33716_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 33720_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 33720_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
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Considering the candidate 33931_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 33931_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
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Considering the candidate 33960_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 33960_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.2") between the two second-epoch detections
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Considering the candidate 33964_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 33964_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 33992_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 33992_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.2") between the two second-epoch detections
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Considering the candidate 34055_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 34055_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
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Considering the candidate 34088_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 34088_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
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Considering the candidate 34134_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 34134_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.6") between the two second-epoch detections
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Considering the candidate 34206_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 34206_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.5") between the two second-epoch detections
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Considering the candidate 34291_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 34291_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.6") between the two second-epoch detections
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Considering the candidate 34294_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 34294_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 34298_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 34298_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (23.0") between the two second-epoch detections
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Considering the candidate 34299_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 34299_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.8") between the two second-epoch detections
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Considering the candidate 34311_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 34311_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.1") between the two second-epoch detections
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Considering the candidate 34356_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 34356_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 34361_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 34361_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 34399_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 34399_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (21.4") between the two second-epoch detections
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Considering the candidate 34433_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 34433_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 34440_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 34440_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
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Considering the candidate 34479_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 34479_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
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Considering the candidate 34527_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 34527_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
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Considering the candidate 34562_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 34562_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
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Considering the candidate 34611_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 34611_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
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Considering the candidate 34635_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 34635_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 34696_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 34696_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.7") between the two second-epoch detections
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Considering the candidate 34700_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 34700_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (21.4") between the two second-epoch detections
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Considering the candidate 34703_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 34703_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 34707_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 34707_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (21.4") between the two second-epoch detections
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Considering the candidate 34754_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 34754_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.5") between the two second-epoch detections
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Considering the candidate 34854_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 34854_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.9") between the two second-epoch detections
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Considering the candidate 34911_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 34911_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 34988_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 34988_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 35024_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 35024_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
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Considering the candidate 35052_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 35052_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
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Considering the candidate 35073_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 35073_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.8") between the two second-epoch detections
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Considering the candidate 35098_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 35098_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 35174_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 35174_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.6") between the two second-epoch detections
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Considering the candidate 35187_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 35187_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 35212_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 35212_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.1") between the two second-epoch detections
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Considering the candidate 35258_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 35258_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.2") between the two second-epoch detections
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Considering the candidate 35270_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 35270_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.4") between the two second-epoch detections
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Considering the candidate 35323_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 35323_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.7") between the two second-epoch detections
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Considering the candidate 35351_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 35351_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.4") between the two second-epoch detections
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Considering the candidate 35388_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 35388_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.4") between the two second-epoch detections
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Considering the candidate 35434_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 35434_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.8") between the two second-epoch detections
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Considering the candidate 35449_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 35449_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 35485_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 35485_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.8") between the two second-epoch detections
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Considering the candidate 35490_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 35490_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (21.4") between the two second-epoch detections
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Considering the candidate 35517_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 35517_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (21.4") between the two second-epoch detections
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Considering the candidate 35634_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 35634_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (23.1") between the two second-epoch detections
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Considering the candidate 35712_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 35712_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 35759_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 35759_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
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Considering the candidate 35760_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 35760_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 35807_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 35807_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (23.2") between the two second-epoch detections
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Considering the candidate 35819_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 35819_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 35833_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 35833_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.9") between the two second-epoch detections
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Considering the candidate 35850_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 35850_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.2") between the two second-epoch detections
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Considering the candidate 35851_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 35851_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
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Considering the candidate 35877_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 35877_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (23.1") between the two second-epoch detections
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Considering the candidate 35952_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 35952_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 35978_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 35978_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.5") between the two second-epoch detections
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Considering the candidate 36052_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 36052_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.5") between the two second-epoch detections
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Considering the candidate 36149_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 36149_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 36176_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 36176_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.7") between the two second-epoch detections
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Considering the candidate 36181_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 36181_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (21.4") between the two second-epoch detections
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Considering the candidate 36196_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 36196_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 36209_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 36209_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.6") between the two second-epoch detections
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Considering the candidate 36239_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 36239_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.8") between the two second-epoch detections
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Considering the candidate 36244_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 36244_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (21.4") between the two second-epoch detections
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Considering the candidate 36245_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 36245_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 36253_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 36253_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.8") between the two second-epoch detections
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Considering the candidate 36258_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 36258_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.9") between the two second-epoch detections
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Considering the candidate 36268_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 36268_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
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Considering the candidate 36291_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 36291_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.1") between the two second-epoch detections
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Considering the candidate 36415_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 36415_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
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Considering the candidate 36432_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 36432_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
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Considering the candidate 36441_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 36441_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.6") between the two second-epoch detections
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Considering the candidate 36443_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
Preparing report for the candidate 36443_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
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Considering the candidate 36456_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 36456_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.7") between the two second-epoch detections
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Considering the candidate 36474_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 36474_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 36530_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 36530_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.7") between the two second-epoch detections
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Considering the candidate 36532_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 36532_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
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Considering the candidate 36563_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 36563_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.8") between the two second-epoch detections
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Considering the candidate 36583_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 36583_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.1") between the two second-epoch detections
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Considering the candidate 36650_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 36650_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 36671_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 36671_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (21.4") between the two second-epoch detections
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Considering the candidate 36710_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 36710_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 36726_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 36726_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.4") between the two second-epoch detections
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Considering the candidate 36731_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 36731_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (21.2") between the two second-epoch detections
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Considering the candidate 36818_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 36818_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
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Considering the candidate 36840_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 36840_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.8") between the two second-epoch detections
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Considering the candidate 36880_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 36880_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.3") between the two second-epoch detections
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Considering the candidate 36898_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 36898_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.7") between the two second-epoch detections
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Considering the candidate 36903_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 36903_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.4") between the two second-epoch detections
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Considering the candidate 36951_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 36951_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 36952_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 36952_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.5") between the two second-epoch detections
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Considering the candidate 37008_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 37008_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 37034_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 37034_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.1") between the two second-epoch detections
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Considering the candidate 37049_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 37049_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.7") between the two second-epoch detections
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Considering the candidate 37075_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 37075_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
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Considering the candidate 37155_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 37155_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
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Considering the candidate 37160_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 37160_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
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Considering the candidate 37217_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 37217_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.2") between the two second-epoch detections
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Considering the candidate 37227_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 37227_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.1") between the two second-epoch detections
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Considering the candidate 37280_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 37280_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 37319_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 37319_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 37323_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 37323_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
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Considering the candidate 37350_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 37350_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.6") between the two second-epoch detections
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Considering the candidate 37351_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 37351_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 37360_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 37360_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
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Considering the candidate 37412_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 37412_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
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Considering the candidate 37496_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 37496_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (22.5") between the two second-epoch detections
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Considering the candidate 37519_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 37519_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 37532_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 37532_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
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Considering the candidate 37584_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 37584_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
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Considering the candidate 37595_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 37595_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (21.3") between the two second-epoch detections
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Considering the candidate 15469_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 15469_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks
Rejecting candidate due to large distance (21.7") between the two second-epoch detections
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Considering the candidate 08030_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391
The candidate 08030_fd_Psc-08-Q2b1x1_2026-10-07_03-54-52_20.00sec_-0.00C_LIGHT_0391 did not pass the final checks