This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC
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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461136.9256,13.38,0.05,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
target 20260406.4256 13.38CV 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
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 06.4256* 21 07 02.86 +16 35 10.4 13.7 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1763792027354203776,2461136.9256,13.72,0.05,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
Gaia DR3 1763792027354203776 20260406.4256 13.72CV 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: 2461036.54134825 27.12.2025 00:59:22.489 /data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits
First image: 2461036.54134825 27.12.2025 00:59:22.489 /data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits
Last image: 2461136.92583818 06.04.2026 10:13:02.419 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 8
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.02
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: 5 seconds
Number of parallel threads: 24
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
Total objects detected (at least 2 times): 11131
Objects passed selection criteria: 11084
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 8166.5
Average stars matched: 7317.25 (89.6008 %)
Memory usage VmPeak: 115580 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 6 05:23:04 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: 2461036.54134825 27.12.2025 00:59:22.489 /data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits
First image: 2461036.54134825 27.12.2025 00:59:22.489 /data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits
Last image: 2461136.92583818 06.04.2026 10:13:02.419 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 65
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.66
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: 35 seconds
Number of parallel threads: 24
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
Total objects detected (at least 2 times): 82619
Objects passed selection criteria: 82354
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 61674.8
Average stars matched: 55200.8 (89.503 %)
Memory usage VmPeak: 1925864 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 6 05:24:59 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 --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits
SExtractor catalog cache: saved Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits.cat to cache
SExtractor catalog cache: saved Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.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/Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461136.92527737
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_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits exists and is non-empty
Saving wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits to local_wcs_cache/
'wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits' -> 'local_wcs_cache/wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits'
wcs_Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits exists and is non-empty
Saving wcs_Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits to local_wcs_cache/
'wcs_Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits' -> 'local_wcs_cache/wcs_Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits'
wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits exists and is non-empty
Saving wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits to local_wcs_cache/
'wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits' -> 'local_wcs_cache/wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits'
wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits exists and is non-empty
Saving wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits to local_wcs_cache/
'wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits' -> 'local_wcs_cache/wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 21:19:58.702 +13:59:25.99
Second-epoch image center 21:20:00.457 +13:59:59.73
Angular distance between the image centers 0.0118 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 21:19:58.702 +13:59:25.99
Second-epoch image center 21:19:58.842 +14:00:09.61
Angular distance between the image centers 0.0121 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 21:20:00.457 +13:59:59.73
Second-epoch second image center 21:19:58.842 +14:00:09.61
Angular distance between the image centers 0.00708 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits &> /tmp/tmp.jnzB25qNBs
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits &> /tmp/tmp.Im5ZFHzAc0
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits &> /tmp/tmp.0Ztwigyir8
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits &> /tmp/tmp.6e83JKy4CO
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits
Calibrating the magnitude scale
Found non-empty wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.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_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits and wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits.cat
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_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits and wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits.cat
Found non-empty wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits and wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits.cat
The reference image (wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits) and catalog (wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits.cat) found
'wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits.cat' -> 'wcsmag.cat'
Read 13427 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 311.7609 to 328.3279 deg, Dec +8.6053 to +19.2832 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 311.7609 to 328.3279 deg, Dec 8.6053 to 19.2832 deg
Loaded 10893 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): 8368 out of 8847 total matches.
Matched with Tycho-2 8847 out of 13427 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.914198
a=0.000000 b=1.000000 c=22.914198
From vast_summary.log: estimated ref. image limiting mag.: -8.02
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.89
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.89
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits
2.3 pix Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits
2.5 pix fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits
2.5 pix fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits
Limiting magnitude estimates:
14.9 mag. Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits
14.9 mag. Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits
14.1 mag. fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits
14.1 mag. fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 11.4 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.jnzB25qNBs (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits' -> 'wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits
WCS_IMAGE_NAME=wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits
WCS-calibrated image found: wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits
Checking if the catalog wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits.cat corresponding to the image wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits alredy exist and is non-empty...
Catalog wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits.cat corresponding to the image wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits
WCS catalog name: wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1001, passed=13427
Got 13427 stars (including 12409 good ones) from the SExtractor catalog wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits.cat
util/solve_plate_with_UCAC5 got 13427 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 923 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 13006 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 13006 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
WARNING: Accuracy estimation diagnostic: 947 matched stars entering correct_measured_positions(), 13006 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 947 stars left (next iteration limit 1041)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits -region wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.Im5ZFHzAc0 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits' -> 'wcs_Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits
WCS_IMAGE_NAME=wcs_Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits
WCS-calibrated image found: wcs_Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits
Checking if the catalog wcs_Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits.cat corresponding to the image wcs_Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits alredy exist and is non-empty...
Catalog wcs_Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits.cat corresponding to the image wcs_Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits
WCS catalog name: wcs_Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1021, passed=13439
Got 13439 stars (including 12391 good ones) from the SExtractor catalog wcs_Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits.cat
util/solve_plate_with_UCAC5 got 13439 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 911 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 12849 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 12854 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
WARNING: Accuracy estimation diagnostic: 941 matched stars entering correct_measured_positions(), 12854 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 941 stars left (next iteration limit 1035)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits -region wcs_Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.0Ztwigyir8 (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_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.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_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits
WCS_IMAGE_NAME=wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits
WCS-calibrated image found: wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits
Checking if the catalog wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits.cat corresponding to the image wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits.cat corresponding to the image wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits
WCS catalog name: wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=585, passed=8170
Got 8170 stars (including 7578 good ones) from the SExtractor catalog wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits.cat
util/solve_plate_with_UCAC5 got 8170 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.9'
Seting catalog search parameters based on the expected field of view 938.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013040 (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 0.010432 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 908 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 7934 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 7934 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
WARNING: Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 7934 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.63"
Excluding outliers - 936 stars left (next iteration limit 1029)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits -region wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.6e83JKy4CO (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_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.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_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits
WCS_IMAGE_NAME=wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits
WCS-calibrated image found: wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits
Checking if the catalog wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits.cat corresponding to the image wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits.cat corresponding to the image wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits
WCS catalog name: wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=551, passed=8275
Got 8275 stars (including 7719 good ones) from the SExtractor catalog wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits.cat
util/solve_plate_with_UCAC5 got 8275 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.9'
Seting catalog search parameters based on the expected field of view 938.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013040 (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 0.010432 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 914 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.58"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 8026 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 8024 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
WARNING: Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 8024 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.62"
Excluding outliers - 936 stars left (next iteration limit 1029)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits -region wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits'
Saving fully-calibrated image wcs_Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/wcs_Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits'
Saving fully-calibrated image wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits'
Saving fully-calibrated image wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits'
Preparing the HTML report for the field Peg-08-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21034_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
The candidate 21034_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418 did not pass the final checks
**** FOUND 21:13:11.56 +12:48:05.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21216_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
The candidate 21216_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418 did not pass the final checks
**** FOUND 21:31:03.94 +11:09:15.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01536_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
The candidate 01536_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418 did not pass the final checks
**** FOUND 21:29:22.77 +18:09:55.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06616_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
The candidate 06616_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418 did not pass the final checks
**** FOUND 21:20:59.85 +14:26:59.5 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Peg-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 --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits
SExtractor catalog cache: saved Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits.cat to cache
SExtractor catalog cache: saved Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits
Creating symlink local_wcs_cache/wcs_Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits
Creating symlink local_wcs_cache/wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits
Creating symlink local_wcs_cache/wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits exists and is non-empty
wcs_Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits exists and is non-empty
wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits exists and is non-empty
wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 21:19:58.702 +13:59:25.99
Second-epoch image center 21:20:00.457 +13:59:59.73
Angular distance between the image centers 0.0118 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 21:19:58.702 +13:59:25.99
Second-epoch image center 21:19:58.842 +14:00:09.61
Angular distance between the image centers 0.0121 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 21:20:00.457 +13:59:59.73
Second-epoch second image center 21:19:58.842 +14:00:09.61
Angular distance between the image centers 0.00708 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits &> /tmp/tmp.FUKC1Y8Wbr
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits &> /tmp/tmp.h9SO1OmInX
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits &> /tmp/tmp.RCWuox2Zsv
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits &> /tmp/tmp.nJ3GXQdXcb
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits
Calibrating the magnitude scale
Found non-empty wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.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_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits and wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits.cat
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_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits and wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits.cat
Found non-empty wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits and wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits.cat
The reference image (wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits) and catalog (wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits.cat) found
'wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits.cat' -> 'wcsmag.cat'
Read 97715 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 311.7453 to 328.3404 deg, Dec +8.5707 to +19.2838 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 311.7453 to 328.3404 deg, Dec 8.5707 to 19.2838 deg
Loaded 10955 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): 7910 out of 9536 total matches.
Matched with Tycho-2 9536 out of 97715 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.741692
a=0.000000 b=1.000000 c=22.741692
From vast_summary.log: estimated ref. image limiting mag.: -7.66
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.08
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.08
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 50 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits
2.1 pix Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits
2.4 pix fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits
2.4 pix fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits
Limiting magnitude estimates:
15.1 mag. Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits
15.1 mag. Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits
14.3 mag. fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits
14.3 mag. fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 13.8 (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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.FUKC1Y8Wbr (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits' -> 'wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits
WCS_IMAGE_NAME=wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits
WCS-calibrated image found: wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits
Checking if the catalog wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits.cat corresponding to the image wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits alredy exist and is non-empty...
Catalog wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits.cat corresponding to the image wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits
WCS catalog name: wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits.cat
SExtractor catalog parsing summary: zero_flux=6, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=24, blended=7308, passed=97685
Got 97685 stars (including 90194 good ones) from the SExtractor catalog wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits.cat
util/solve_plate_with_UCAC5 got 97685 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 913 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 94047 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 94050 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
WARNING: Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 94048 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 946 stars left (next iteration limit 1040)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits -region wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.h9SO1OmInX (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits' -> 'wcs_Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits
WCS_IMAGE_NAME=wcs_Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits
WCS-calibrated image found: wcs_Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits
Checking if the catalog wcs_Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits.cat corresponding to the image wcs_Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits alredy exist and is non-empty...
Catalog wcs_Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits.cat corresponding to the image wcs_Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits
WCS catalog name: wcs_Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=27, blended=7285, passed=98170
Got 98170 stars (including 90714 good ones) from the SExtractor catalog wcs_Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits.cat
util/solve_plate_with_UCAC5 got 98170 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 915 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 93863 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 93865 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
WARNING: Accuracy estimation diagnostic: 946 matched stars entering correct_measured_positions(), 93863 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 946 stars left (next iteration limit 1040)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits -region wcs_Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.RCWuox2Zsv (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_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.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_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits
WCS_IMAGE_NAME=wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits
WCS-calibrated image found: wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits
Checking if the catalog wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits.cat corresponding to the image wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits.cat corresponding to the image wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits
WCS catalog name: wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=3555, passed=55708
Got 55708 stars (including 52091 good ones) from the SExtractor catalog wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits.cat
util/solve_plate_with_UCAC5 got 55708 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.9'
Seting catalog search parameters based on the expected field of view 938.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013040 (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 0.010432 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 896 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 53847 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 53844 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
WARNING: Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 53844 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.59"
Excluding outliers - 934 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits -region wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.nJ3GXQdXcb (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_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.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_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits
WCS_IMAGE_NAME=wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits
WCS-calibrated image found: wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits
Checking if the catalog wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits.cat corresponding to the image wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits.cat corresponding to the image wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits
WCS catalog name: wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=3490, passed=55046
Got 55046 stars (including 51488 good ones) from the SExtractor catalog wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits.cat
util/solve_plate_with_UCAC5 got 55046 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.9'
Seting catalog search parameters based on the expected field of view 938.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013040 (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 0.010432 (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
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 900 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 53183 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 53185 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
WARNING: Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 53185 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Excluding outliers - 936 stars left (next iteration limit 1029)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits -region wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.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_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/wcs_Peg-08-Q2b1x1_2025-12-26_18-59-22_20.00sec_-14.90C_LIGHT_0000.fits
Saving fully-calibrated image wcs_Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.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_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/wcs_Peg-08-Q2b1x1_2025-12-26_19-00-06_20.00sec_-15.00C_LIGHT_0001.fits
Saving fully-calibrated image wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.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_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-12-13_20.00sec_-4.90C_LIGHT_0417.fits
Saving fully-calibrated image wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.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_2026-04-06_CI_Peg-08-Q2b1x1_051441_TTUQ2b1x1_24719_HZUu7fLC/wcs_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418.fits
Preparing the HTML report for the field Peg-08-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out114531.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out114533.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out114535.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out114537.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out114541.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out114544.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out121475.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125522.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out126061.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out127895.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out130871.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out131156.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out126395.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out127457.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 19s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 114531_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
The candidate 114531_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418 did not pass the final checks
**** FOUND 21:06:35.23 +15:59:13.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 1.279 1763733581438799488 316.64714411064 +15.98686526686 13.9211 13.1166 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.279#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 114533_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
The candidate 114533_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418 did not pass the final checks
**** FOUND 21:18:56.40 +17:49:32.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 1.486 1785414645068432000 319.73507554606 +17.82517692536 14.2410 13.7658 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.486#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 114535_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
The candidate 114535_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418 did not pass the final checks
**** FOUND 21:09:10.43 +14:52:53.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.83, MAG_FAINT_SEARCH_LIMIT=14.81)GAIADR2_OUTPUT=# 1.521 1760044921790043776 317.29357715461 +14.88185115443 13.9008 13.2844 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.521#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 114536_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
The candidate 114536_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418 did not pass the final checks
**** FOUND 21:29:33.63 +16:37:33.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 114537_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
The candidate 114537_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418 did not pass the final checks
**** FOUND 21:35:50.57 +13:41:26.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)
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Considering the candidate 114540_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
The candidate 114540_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418 did not pass the final checks
**** FOUND 21:14:47.46 +16:17:50.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 114541_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
The candidate 114541_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418 did not pass the final checks
**** FOUND 21:05:36.91 +16:37:33.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 1.783 1763836484559344640 316.40430579396 +16.62605062900 13.5657 12.8508 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.783#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 114542_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
The candidate 114542_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418 did not pass the final checks
**** FOUND 21:11:21.41 +13:21:06.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 114544_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
The candidate 114544_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418 did not pass the final checks
**** FOUND 21:08:53.70 +10:22:28.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)
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Considering the candidate 114546_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
The candidate 114546_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418 did not pass the final checks
**** FOUND 21:13:41.57 +17:59:20.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 114548_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
The candidate 114548_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418 did not pass the final checks
**** FOUND 21:07:29.99 +12:08:34.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 118468_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
The candidate 118468_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418 did not pass the final checks
**** FOUND 21:25:48.68 +15:35:23.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 119524_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
The candidate 119524_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418 did not pass the final checks
**** FOUND 21:18:31.03 +17:42:42.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 120277_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
The candidate 120277_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418 did not pass the final checks
**** FOUND 21:14:40.79 +16:29:15.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 120566_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
The candidate 120566_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418 did not pass the final checks
**** FOUND 21:29:56.16 +12:12:30.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 120585_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
The candidate 120585_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418 did not pass the final checks
**** FOUND 21:14:34.41 +11:56:47.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 120598_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
The candidate 120598_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418 did not pass the final checks
**** FOUND 21:18:35.55 +11:35:32.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 120954_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
The candidate 120954_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418 did not pass the final checks
**** FOUND 21:21:38.17 +17:09:45.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 121475_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
The candidate 121475_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418 did not pass the final checks
**** FOUND 21:08:18.26 +13:25:29.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 1.121 1759048077060266368 317.07578998031 +13.42490276525 12.9171 12.4544 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.121#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 121714_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
The candidate 121714_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418 did not pass the final checks
**** FOUND 21:11:51.55 +12:56:03.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 121767_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
The candidate 121767_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418 did not pass the final checks
**** FOUND 21:12:08.85 +11:48:29.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 122417_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
The candidate 122417_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418 did not pass the final checks
**** FOUND 21:13:51.02 +17:15:20.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 124094_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
The candidate 124094_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418 did not pass the final checks
**** FOUND 21:21:24.91 +17:10:37.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 124098_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
The candidate 124098_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418 did not pass the final checks
**** FOUND 21:04:09.57 +10:01:10.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 124882_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
The candidate 124882_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418 did not pass the final checks
**** FOUND 21:07:39.90 +15:40:30.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 124938_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
The candidate 124938_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418 did not pass the final checks
**** FOUND 21:18:28.50 +17:44:12.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125012_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
The candidate 125012_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418 did not pass the final checks
**** FOUND 21:15:57.13 +10:42:08.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125522_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
The candidate 125522_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418 did not pass the final checks
**** FOUND 21:02:59.11 +16:12:56.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 3.712 1763435751227360512 315.74734621198 +16.21588889720 13.9158 13.3564 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.712#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 126006_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
The candidate 126006_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418 did not pass the final checks
**** FOUND 21:02:11.94 +14:27:26.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 126061_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
The candidate 126061_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418 did not pass the final checks
**** FOUND 21:08:41.29 +15:41:47.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 1.675 1760684292098287616 317.17157203772 +15.69641844520 13.5638 12.8659 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.675#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 126234_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
The candidate 126234_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418 did not pass the final checks
**** FOUND 21:36:38.26 +15:41:29.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 126395_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
Preparing report for the candidate 126395_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
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Considering the candidate 126407_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
The candidate 126407_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418 did not pass the final checks
**** FOUND 21:06:26.78 +13:07:46.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 126554_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
The candidate 126554_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418 did not pass the final checks
**** FOUND 21:07:19.65 +14:53:27.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 127457_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
Preparing report for the candidate 127457_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
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Considering the candidate 127895_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
The candidate 127895_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418 did not pass the final checks
**** FOUND 21:10:37.26 +16:50:11.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 4.940 1763907063757807488 317.65654237442 +16.83698276163 13.9411 13.2585 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.940#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 128577_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
The candidate 128577_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418 did not pass the final checks
**** FOUND 21:30:52.93 +12:57:20.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 129139_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
The candidate 129139_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418 did not pass the final checks
**** FOUND 21:10:37.11 +16:50:41.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130871_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
The candidate 130871_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418 did not pass the final checks
**** FOUND 21:07:27.79 +16:51:58.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)GAIADR2_OUTPUT=# 0.828 1763943485080676480 316.86589073939 +16.86640399360 14.5323 14.0320 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.828#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131156_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
The candidate 131156_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418 did not pass the final checks
**** FOUND 21:03:49.46 +12:31:22.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)GAIADR2_OUTPUT=# 1.019 1757465746685745664 315.95603536821 +12.52327911501 14.5587 13.9529 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.019#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131950_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
The candidate 131950_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418 did not pass the final checks
**** FOUND 21:11:18.27 +13:21:45.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 86932_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
The candidate 86932_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418 did not pass the final checks
**** FOUND 21:04:59.31 +11:29:23.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 10502_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
The candidate 10502_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418 did not pass the final checks
**** FOUND 21:29:22.75 +18:09:55.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 28017_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
The candidate 28017_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418 did not pass the final checks
**** FOUND 21:14:24.24 +16:28:21.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 87163_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
The candidate 87163_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418 did not pass the final checks
**** FOUND 21:13:11.57 +12:48:05.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 80004_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
The candidate 80004_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418 did not pass the final checks
Rejecting candidate due to large distance (25.8") between the two second-epoch detections
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Considering the candidate 109419_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
The candidate 109419_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418 did not pass the final checks
Rejecting candidate due to large distance (24.6") between the two second-epoch detections
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Considering the candidate 83962_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
The candidate 83962_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418 did not pass the final checks
**** FOUND 21:31:03.96 +11:09:15.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58525_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
The candidate 58525_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418 did not pass the final checks
**** FOUND 21:07:13.06 +13:21:21.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 46914_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418
The candidate 46914_fd_Peg-08-Q2b1x1_2026-04-06_05-13-02_20.00sec_-4.90C_LIGHT_0418 did not pass the final checks