This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr
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
ASAS J223201+2019.9,2461125.9748,11.04,0.05,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
ASAS J223201+2019.9 20260326.4748 11.04CV 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
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:32:01.12 +20:19:54.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20_00sec_-15_00C_LIGHT_0018_fits__*pix.png resample_wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20_00sec_-14_90C_LIGHT_0696_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20_00sec_-15_00C_LIGHT_0018_fits__*pix.png resample_wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20_00sec_-15_00C_LIGHT_0695_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20_00sec_-15_00C_LIGHT_0018_fits__*pix.png resample_wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20_00sec_-14_90C_LIGHT_0696_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20_00sec_-15_00C_LIGHT_0018_fits__*pix.png resample_wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20_00sec_-15_00C_LIGHT_0695_fits__*pix.png animation_v2.gif
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
Gaia DR3 1878546475397491456,2461125.9748,13.55,0.05,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 1878546475397491456 20260326.4748 13.55CV 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
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:17:59.35 +24:09:07.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20_00sec_-15_00C_LIGHT_0018_fits__*pix.png resample_wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20_00sec_-14_90C_LIGHT_0696_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20_00sec_-15_00C_LIGHT_0018_fits__*pix.png resample_wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20_00sec_-15_00C_LIGHT_0695_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20_00sec_-15_00C_LIGHT_0018_fits__*pix.png resample_wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20_00sec_-14_90C_LIGHT_0696_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20_00sec_-15_00C_LIGHT_0018_fits__*pix.png resample_wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20_00sec_-15_00C_LIGHT_0695_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461036.55357920 27.12.2025 01:16:59.243 /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
First image: 2461036.55357920 27.12.2025 01:16:59.243 /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
Last image: 2461125.97504206 26.03.2026 11:23:53.634 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.93
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 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): 11421
Objects passed selection criteria: 11385
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 9253
Average stars matched: 8644 (93.4184 %)
Memory usage VmPeak: 116340 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 26 06:33:22 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: 2461036.55357920 27.12.2025 01:16:59.243 /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
First image: 2461036.55357920 27.12.2025 01:16:59.243 /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
Last image: 2461125.97504206 26.03.2026 11:23:53.634 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 54
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.59
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: 37 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): 75814
Objects passed selection criteria: 75626
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 63423.2
Average stars matched: 59066.5 (93.1307 %)
Memory usage VmPeak: 1901940 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 26 06:34:40 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-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits
SExtractor catalog cache: saved Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits.cat to cache
SExtractor catalog cache: saved Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.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-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.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: 2461125.97450391
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits exists and is non-empty
Saving wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits to local_wcs_cache/
'wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits' -> 'local_wcs_cache/wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits'
wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits exists and is non-empty
Saving wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits to local_wcs_cache/
'wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits' -> 'local_wcs_cache/wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits'
wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits exists and is non-empty
Saving wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits to local_wcs_cache/
'wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits' -> 'local_wcs_cache/wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits'
wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits exists and is non-empty
Saving wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits to local_wcs_cache/
'wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits' -> 'local_wcs_cache/wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.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 22:09:14.257 +21:59:49.67
Second-epoch image center 22:09:12.590 +21:59:23.23
Angular distance between the image centers 0.01 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 22:09:14.257 +21:59:49.67
Second-epoch image center 22:09:13.553 +21:58:59.80
Angular distance between the image centers 0.01 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 22:09:12.590 +21:59:23.23
Second-epoch second image center 22:09:13.553 +21:58:59.80
Angular distance between the image centers 0.00750 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-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits &> /tmp/tmp.R32kQRtDXW
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits &> /tmp/tmp.BKMlA7QPBR
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits &> /tmp/tmp.Ezc9GCWc9d
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits &> /tmp/tmp.3rvO3CK6kP
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits
Calibrating the magnitude scale
Found non-empty wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.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-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits and wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.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-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits and wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits.cat
Found non-empty wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits and wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits.cat
The reference image (wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits) and catalog (wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits.cat) found
'wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits.cat' -> 'wcsmag.cat'
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
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 8532 out of 12915 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.918847
a=0.000000 b=1.000000 c=22.918847
From vast_summary.log: estimated ref. image limiting mag.: -7.93
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.99
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.99
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.4 pix Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
2.4 pix Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits
2.5 pix fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits
2.5 pix fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits
Limiting magnitude estimates:
15.0 mag. Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
15.0 mag. Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits
14.5 mag. fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits
14.5 mag. fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 11.7 (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.R32kQRtDXW (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-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.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_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.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-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.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-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits' -> 'wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
WCS_IMAGE_NAME=wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
WCS-calibrated image found: wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
Checking if the catalog wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits.cat corresponding to the image wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits alredy exist and is non-empty...
Catalog wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits.cat corresponding to the image wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
WCS catalog name: wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1046, passed=12915
Got 12915 stars (including 11858 good ones) from the SExtractor catalog wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits.cat
util/solve_plate_with_UCAC5 got 12915 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
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...
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.42"
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits -region wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.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.BKMlA7QPBR (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-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.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_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.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-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.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-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits' -> 'wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits
WCS_IMAGE_NAME=wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits
WCS-calibrated image found: wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits
Checking if the catalog wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits.cat corresponding to the image wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits alredy exist and is non-empty...
Catalog wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits.cat corresponding to the image wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits
WCS catalog name: wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1022, passed=12932
Got 12932 stars (including 11893 good ones) from the SExtractor catalog wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits.cat
util/solve_plate_with_UCAC5 got 12932 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
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...
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.43"
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits -region wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.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.Ezc9GCWc9d (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_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.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_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits
WCS_IMAGE_NAME=wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits
WCS-calibrated image found: wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits
Checking if the catalog wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits.cat corresponding to the image wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits.cat corresponding to the image wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits
WCS catalog name: wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=603, passed=9392
Got 9392 stars (including 8778 good ones) from the SExtractor catalog wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits.cat
util/solve_plate_with_UCAC5 got 9392 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.2'
Seting catalog search parameters based on the expected field of view 939.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013044 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010436 (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...
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.49"
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 955 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits -region wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.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.3rvO3CK6kP (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_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.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_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits
WCS_IMAGE_NAME=wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits
WCS-calibrated image found: wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits
Checking if the catalog wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits.cat corresponding to the image wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits.cat corresponding to the image wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits
WCS catalog name: wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=524, passed=9232
Got 9232 stars (including 8704 good ones) from the SExtractor catalog wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits.cat
util/solve_plate_with_UCAC5 got 9232 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.2'
Seting catalog search parameters based on the expected field of view 939.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013044 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010436 (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...
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.51"
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...
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.51"
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits -region wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.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-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits'
Saving fully-calibrated image wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits'
Saving fully-calibrated image wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits'
Saving fully-calibrated image wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits'
Preparing the HTML report for the field Peg-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out21531.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out08694.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 3s
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 21531_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696
The candidate 21531_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696 did not pass the final checks
**** FOUND 22:09:55.81 +18:47:52.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.38, MAG_FAINT_SEARCH_LIMIT=12.36)GAIADR2_OUTPUT=# 3.089 1776575808531224960 332.48255390338 +18.79869143534 9.8994 8.4504 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.089#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08694_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696
Preparing report for the candidate 08694_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 4s
Prepared the HTML report for the field Peg-05-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 ####
22:32:01.12 +20:19:54.3
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-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits
SExtractor catalog cache: saved Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits.cat to cache
SExtractor catalog cache: saved Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.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-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
Creating symlink local_wcs_cache/wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits
Creating symlink local_wcs_cache/wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits
Creating symlink local_wcs_cache/wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.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-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits exists and is non-empty
wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits exists and is non-empty
wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits exists and is non-empty
wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.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 22:09:14.257 +21:59:49.67
Second-epoch image center 22:09:12.590 +21:59:23.23
Angular distance between the image centers 0.01 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 22:09:14.257 +21:59:49.67
Second-epoch image center 22:09:13.553 +21:58:59.80
Angular distance between the image centers 0.01 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 22:09:12.590 +21:59:23.23
Second-epoch second image center 22:09:13.553 +21:58:59.80
Angular distance between the image centers 0.00750 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-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits &> /tmp/tmp.IOS8oEEWFs
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits &> /tmp/tmp.cKtPZssdiB
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits &> /tmp/tmp.nrPQZFWTmp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits &> /tmp/tmp.whJpW663bS
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits
Calibrating the magnitude scale
Found non-empty wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.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-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits and wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.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-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits and wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits.cat
Found non-empty wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits and wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits.cat
The reference image (wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits) and catalog (wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits.cat) found
'wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits.cat' -> 'wcsmag.cat'
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
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 9018 out of 86189 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.751336
a=0.000000 b=1.000000 c=22.751336
From vast_summary.log: estimated ref. image limiting mag.: -7.59
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.16
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.16
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 44 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
2.2 pix Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits
2.4 pix fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits
2.3 pix fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits
Limiting magnitude estimates:
15.2 mag. Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
15.2 mag. Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits
14.6 mag. fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits
14.7 mag. fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 14.1 (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.IOS8oEEWFs (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-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.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_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.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-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.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-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits' -> 'wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
WCS_IMAGE_NAME=wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
WCS-calibrated image found: wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
Checking if the catalog wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits.cat corresponding to the image wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits alredy exist and is non-empty...
Catalog wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits.cat corresponding to the image wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
WCS catalog name: wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=23, blended=6314, passed=86166
Got 86166 stars (including 79704 good ones) from the SExtractor catalog wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits.cat
util/solve_plate_with_UCAC5 got 86166 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
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...
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.43"
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits -region wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.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.cKtPZssdiB (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-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.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_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.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-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.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-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits' -> 'wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits
WCS_IMAGE_NAME=wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits
WCS-calibrated image found: wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits
Checking if the catalog wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits.cat corresponding to the image wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits alredy exist and is non-empty...
Catalog wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits.cat corresponding to the image wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits
WCS catalog name: wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=34, blended=6394, passed=85906
Got 85906 stars (including 79384 good ones) from the SExtractor catalog wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits.cat
util/solve_plate_with_UCAC5 got 85906 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
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...
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.43"
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits -region wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.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.nrPQZFWTmp (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_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.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_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits
WCS_IMAGE_NAME=wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits
WCS-calibrated image found: wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits
Checking if the catalog wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits.cat corresponding to the image wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits.cat corresponding to the image wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits
WCS catalog name: wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits.cat
SExtractor catalog parsing summary: zero_flux=6, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=3529, passed=59420
Got 59420 stars (including 55841 good ones) from the SExtractor catalog wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits.cat
util/solve_plate_with_UCAC5 got 59420 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.2'
Seting catalog search parameters based on the expected field of view 939.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013044 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010436 (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...
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.47"
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...
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.47"
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits -region wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.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.whJpW663bS (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_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.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_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits
WCS_IMAGE_NAME=wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits
WCS-calibrated image found: wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits
Checking if the catalog wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits.cat corresponding to the image wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits.cat corresponding to the image wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits
WCS catalog name: wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=3423, passed=60483
Got 60483 stars (including 56979 good ones) from the SExtractor catalog wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits.cat
util/solve_plate_with_UCAC5 got 60483 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.2'
Seting catalog search parameters based on the expected field of view 939.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013044 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010436 (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...
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.48"
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits -region wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.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-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.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_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/wcs_Peg-05-Q2b1x1_2025-12-26_19-16-59_20.00sec_-15.00C_LIGHT_0018.fits
Saving fully-calibrated image wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.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_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/wcs_Peg-05-Q2b1x1_2025-12-26_19-18-03_20.00sec_-14.90C_LIGHT_0019.fits
Saving fully-calibrated image wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.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_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-07_20.00sec_-15.00C_LIGHT_0695.fits
Saving fully-calibrated image wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.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_2026-03-26_CI_Peg-05-Q2b1x1_063037_TTUQ2b1x1_11459_pFRXgnNr/wcs_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696.fits
Preparing the HTML report for the field Peg-05-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out102239.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out102242.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out102250.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out102253.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out102256.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out102259.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out102262.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out102263.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103548.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105049.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107983.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out108130.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out108175.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out108200.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out108305.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out108598.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out108613.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out109314.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out109500.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out109541.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out109709.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out110036.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out110080.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out110158.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out111166.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out111916.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112002.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112102.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112200.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112270.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112314.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112324.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out108238.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
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Considering the candidate 102239_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696
The candidate 102239_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696 did not pass the final checks
**** FOUND 22:09:17.64 +22:54:26.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.51, MAG_FAINT_SEARCH_LIMIT=15.49)GAIADR2_OUTPUT=# 1.391 1783022279564876416 332.32317873962 +22.90760944664 14.5933 13.8913 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.391#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 102242_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696
The candidate 102242_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696 did not pass the final checks
**** FOUND 22:10:31.69 +20:40:40.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.37, MAG_FAINT_SEARCH_LIMIT=15.35)GAIADR2_OUTPUT=# 2.747 1781348376190686592 332.63140160120 +20.67847287174 14.7984 14.2779 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.747#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 102250_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696
The candidate 102250_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696 did not pass the final checks
**** FOUND 22:01:40.74 +24:44:52.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.13, MAG_FAINT_SEARCH_LIMIT=15.11)GAIADR2_OUTPUT=# 0.560 1795674188068107392 330.41977338713 +24.74795977619 14.1432 13.6049 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.560#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 102253_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696
The candidate 102253_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696 did not pass the final checks
**** FOUND 22:17:08.27 +22:26:10.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 2.316 1878072929482086272 334.28386155089 +22.43580761302 14.1062 13.3410 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.316#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 102256_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696
The candidate 102256_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696 did not pass the final checks
**** FOUND 21:48:35.19 +22:43:32.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)GAIADR2_OUTPUT=# 1.907 1793512616926288512 327.14642700730 +22.72605269619 13.9403 13.3811 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.907#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 102259_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696
The candidate 102259_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696 did not pass the final checks
**** FOUND 21:54:30.70 +25:54:22.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)
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Considering the candidate 102262_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696
The candidate 102262_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696 did not pass the final checks
**** FOUND 21:59:18.52 +21:29:41.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 0.383 1782583505705792640 329.82707368293 +21.49492293374 13.8032 13.3544 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.383#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 102263_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696
The candidate 102263_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696 did not pass the final checks
**** FOUND 22:24:15.99 +21:07:29.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)GAIADR2_OUTPUT=# 1.261 1874650867043708928 336.06642106453 +21.12518296528 13.6400 13.0859 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.261#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103548_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696
The candidate 103548_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696 did not pass the final checks
**** FOUND 22:14:24.47 +22:05:41.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.77, MAG_FAINT_SEARCH_LIMIT=12.75)GAIADR2_OUTPUT=# 0.641 1781975334040640384 333.60177500026 +22.09466903210 11.5677 11.0844 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.641#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 104514_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696
The candidate 104514_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696 did not pass the final checks
**** FOUND 22:07:43.42 +21:41:17.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 105049_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696
The candidate 105049_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696 did not pass the final checks
**** FOUND 22:26:48.79 +22:48:38.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 0.892 1875472653202594688 336.70318206887 +22.81092070817 12.4391 11.8450 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.892#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106274_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696
The candidate 106274_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696 did not pass the final checks
**** FOUND 22:06:49.80 +25:51:42.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106520_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696
The candidate 106520_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696 did not pass the final checks
**** FOUND 22:30:14.56 +22:26:52.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106556_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696
The candidate 106556_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696 did not pass the final checks
**** FOUND 22:25:34.63 +18:27:31.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 106823_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696
The candidate 106823_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696 did not pass the final checks
**** FOUND 21:52:20.01 +21:18:38.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107657_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696
The candidate 107657_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696 did not pass the final checks
**** FOUND 22:11:18.28 +19:49:18.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107983_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696
The candidate 107983_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696 did not pass the final checks
**** FOUND 21:47:06.24 +23:51:34.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 2.625 1794588111096932352 326.77526285890 +23.85991701998 13.6206 13.1772 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.625#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 108130_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696
The candidate 108130_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696 did not pass the final checks
**** FOUND 21:46:03.99 +20:01:08.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 2.865 1792474403071767552 326.51578747607 +20.01914650263 13.6255 13.0898 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.865#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 108175_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696
The candidate 108175_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696 did not pass the final checks
**** FOUND 22:32:26.99 +21:04:03.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 3.761 1873765176067640832 338.11154412305 +21.06821402605 13.4118 12.7147 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.761#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 108197_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696
The candidate 108197_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696 did not pass the final checks
**** FOUND 21:57:30.51 +23:33:00.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 108200_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696
The candidate 108200_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696 did not pass the final checks
**** FOUND 22:04:52.68 +21:16:24.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 2.431 1781594220118874880 331.21948331477 +21.27414734575 13.6807 13.1048 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.431#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 108238_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696
Preparing report for the candidate 108238_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696
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Considering the candidate 108305_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696
The candidate 108305_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696 did not pass the final checks
**** FOUND 21:46:56.12 +21:19:13.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 3.964 1792900360748184832 326.73384534496 +21.32143448536 13.8319 13.2553 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.964#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 108542_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696
The candidate 108542_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696 did not pass the final checks
**** FOUND 21:59:30.66 +19:19:47.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 108598_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696
The candidate 108598_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696 did not pass the final checks
**** FOUND 22:23:20.88 +21:59:00.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 1.186 1874953404540774400 335.83734934705 +21.98347674577 13.6401 13.3505 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.186#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 108613_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696
The candidate 108613_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696 did not pass the final checks
**** FOUND 21:58:52.17 +21:52:38.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 1.370 1782612780203129728 329.71759792675 +21.87754165623 13.9163 13.2993 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.370#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 108648_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696
The candidate 108648_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696 did not pass the final checks
**** FOUND 22:29:46.05 +20:19:16.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 109314_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696
The candidate 109314_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696 did not pass the final checks
**** FOUND 22:35:08.92 +23:18:14.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 1.281 1875374349991534464 338.78707255344 +23.30428953786 13.6988 13.1136 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.281#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 109500_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696
The candidate 109500_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696 did not pass the final checks
**** FOUND 22:07:01.51 +25:51:51.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 4.677 1891838059148731136 331.75713061403 +25.86541834028 14.0098 13.3572 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.677#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 109541_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696
The candidate 109541_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696 did not pass the final checks
**** FOUND 22:01:23.71 +24:17:50.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 4.266 1795374055752755840 330.34777845448 +24.29804828289 14.0410 13.5356 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.266#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 109709_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696
The candidate 109709_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696 did not pass the final checks
**** FOUND 22:24:51.44 +23:27:52.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 0.707 1878566816362198400 336.21449800873 +23.46451335598 13.8013 13.2683 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.707#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 110036_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696
The candidate 110036_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696 did not pass the final checks
**** FOUND 21:55:16.04 +23:59:59.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)
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Considering the candidate 110080_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696
The candidate 110080_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696 did not pass the final checks
**** FOUND 22:03:43.29 +20:18:46.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 2.757 1779972680986095232 330.93002511281 +20.31355301451 14.3993 13.9618 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.757#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 110158_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696
The candidate 110158_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696 did not pass the final checks
**** FOUND 22:13:54.42 +22:09:52.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 1.858 1781973998306859136 333.47694355965 +22.16495609941 14.0468 13.5898 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.858#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 111166_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696
The candidate 111166_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696 did not pass the final checks
**** FOUND 22:07:53.65 +24:08:18.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)GAIADR2_OUTPUT=# 0.469 1783393364740040832 331.97368416397 +24.13854752706 14.1274 13.4239 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.469#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 111916_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696
The candidate 111916_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696 did not pass the final checks
**** FOUND 21:59:29.88 +23:07:06.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.41, MAG_FAINT_SEARCH_LIMIT=15.39)
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Considering the candidate 112002_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696
The candidate 112002_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696 did not pass the final checks
**** FOUND 21:43:49.44 +23:08:11.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)GAIADR2_OUTPUT=# 1.075 1794441498093264896 325.95608894033 +23.13684289043 14.3079 13.7423 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.075#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 112065_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696
The candidate 112065_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 112102_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696
The candidate 112102_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696 did not pass the final checks
**** FOUND 22:16:17.44 +23:11:27.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)GAIADR2_OUTPUT=# 1.000 1878312863535948544 334.07240617345 +23.19105764099 14.6468 14.2588 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.000#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 112200_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696
The candidate 112200_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696 did not pass the final checks
**** FOUND 21:57:38.68 +19:58:26.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.49, MAG_FAINT_SEARCH_LIMIT=15.47)GAIADR2_OUTPUT=# 1.945 1780652591488769408 329.41105481249 +19.97447453498 14.3833 13.8592 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.945#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 112270_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696
The candidate 112270_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696 did not pass the final checks
**** FOUND 21:55:23.10 +19:53:43.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.44, MAG_FAINT_SEARCH_LIMIT=15.42)GAIADR2_OUTPUT=# 1.147 1780636506836153216 328.84595475802 +19.89562838397 14.5873 14.0988 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.147#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 112314_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696
The candidate 112314_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696 did not pass the final checks
**** FOUND 22:01:05.37 +22:11:34.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.62, MAG_FAINT_SEARCH_LIMIT=15.60)GAIADR2_OUTPUT=# 1.183 1782645593753111424 330.27209098161 +22.19300272747 14.7655 14.1214 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.183#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 112324_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696
The candidate 112324_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696 did not pass the final checks
**** FOUND 22:06:00.85 +22:26:14.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.68, MAG_FAINT_SEARCH_LIMIT=15.66)GAIADR2_OUTPUT=# 2.474 1782934215555334272 331.50285246648 +22.43770232215 14.5481 13.8458 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.474#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 85917_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696
The candidate 85917_fd_Peg-05-Q2b1x1_2026-03-26_06-23-53_20.00sec_-14.90C_LIGHT_0696 did not pass the final checks