This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 03 29.4659 2461128.9659 13.86 22:11:13.65 +20:03:34.2
79.25895 -28.91542 galactic Peg Second-epoch detections are separated by 3.2" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 22:11:13.65 +20:03:34.2 (user input) | T | P | (position from user input) J-Ks=0.353+/-0.037 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461128.9659,13.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260329.4659 13.86CV 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_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:11:13.65 +20:03:34.2 ;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_2026-03-29_06-11-16_20_00sec_-15_00C_LIGHT_0430_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_2026-03-29_06-10-17_20_00sec_-14_90C_LIGHT_0429_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_2026-03-29_06-11-16_20_00sec_-15_00C_LIGHT_0430_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_2026-03-29_06-10-17_20_00sec_-14_90C_LIGHT_0429_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
V0505 Peg,2461128.9659,12.77,0.05,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
V0505 Peg 20260329.4659 12.77CV 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_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:09:19.10 +19:43:58.1 ;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_2026-03-29_06-11-16_20_00sec_-15_00C_LIGHT_0430_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_2026-03-29_06-10-17_20_00sec_-14_90C_LIGHT_0429_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_2026-03-29_06-11-16_20_00sec_-15_00C_LIGHT_0430_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_2026-03-29_06-10-17_20_00sec_-14_90C_LIGHT_0429_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: 2461128.96627487 29.03.2026 11:11:16.149 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.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: 5 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 11263
Objects passed selection criteria: 11217
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 8760
Average stars matched: 8185 (93.4361 %)
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 Sun Mar 29 06:14:29 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: 2461128.96627487 29.03.2026 11:11:16.149 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 69
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: 27 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): 75586
Objects passed selection criteria: 75416
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: 62261.8
Average stars matched: 57862 (92.9335 %)
Memory usage VmPeak: 2023324 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 Sun Mar 29 06:15:38 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_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.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_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.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: 2461128.96559174
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
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
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_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits exists and is non-empty
Saving wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits to local_wcs_cache/
'wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits' -> 'local_wcs_cache/wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits'
wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.fits exists and is non-empty
Saving wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.fits to local_wcs_cache/
'wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.fits' -> 'local_wcs_cache/wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.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 22:09:08.672 +21:57:24.17
Angular distance between the image centers 0.05 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 22:09:07.628 +21:57:47.04
Angular distance between the image centers 0.04 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 22:09:08.672 +21:57:24.17
Second-epoch second image center 22:09:07.628 +21:57:47.04
Angular distance between the image centers 0.00753 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.JHezDqcMQc
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.FOqif2WPns
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_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits &> /tmp/tmp.oZQUb6LWwJ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.fits &> /tmp/tmp.Y92vlouSO0
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.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
2.4 pix fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits
2.4 pix fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.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
14.4 mag. fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits
14.4 mag. fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 11.6 (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.JHezDqcMQc (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_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/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.FOqif2WPns (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_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/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.oZQUb6LWwJ (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_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.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_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits
WCS_IMAGE_NAME=wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits
WCS-calibrated image found: wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits
Checking if the catalog wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits.cat corresponding to the image wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits.cat corresponding to the image wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.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_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits
WCS catalog name: wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits.cat
SExtractor catalog parsing summary: zero_flux=1, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=468, passed=8050
Got 8050 stars (including 7576 good ones) from the SExtractor catalog wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits.cat
util/solve_plate_with_UCAC5 got 8050 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.4'
Seting catalog search parameters based on the expected field of view 939.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013047 (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 0.010438 (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: 0.48"
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 956 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: 0.50"
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_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits -region wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.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.Y92vlouSO0 (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_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.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_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.fits
WCS_IMAGE_NAME=wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.fits
WCS-calibrated image found: wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.fits
Checking if the catalog wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.fits.cat corresponding to the image wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.fits.cat corresponding to the image wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.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_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.fits
WCS catalog name: wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.fits.cat
SExtractor catalog parsing summary: zero_flux=4, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=547, passed=8208
Got 8208 stars (including 7651 good ones) from the SExtractor catalog wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.fits.cat
util/solve_plate_with_UCAC5 got 8208 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.3'
Seting catalog search parameters based on the expected field of view 939.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013046 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010437 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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: 0.49"
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 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.50"
Estimated accuracy of the plate solution: 0.52"
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_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.fits -region wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.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_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/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_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/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_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits'
Saving fully-calibrated image wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.fits'
Preparing the HTML report for the field Peg-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21587_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 21587_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 22:09:55.82 +18:47:51.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08694_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 08694_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 22:32:01.13 +20:19:54.4 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Peg-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 ####
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_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.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_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.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_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits
Creating symlink local_wcs_cache/wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.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_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits exists and is non-empty
wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.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 22:09:08.672 +21:57:24.17
Angular distance between the image centers 0.05 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 22:09:07.628 +21:57:47.04
Angular distance between the image centers 0.04 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 22:09:08.672 +21:57:24.17
Second-epoch second image center 22:09:07.628 +21:57:47.04
Angular distance between the image centers 0.00753 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.LmUUyrn7T7
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.6STK0KggMy
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_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits &> /tmp/tmp.ZMxBiMqrTe
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.fits &> /tmp/tmp.T64yhxwJ6r
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.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 56 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
2.2 pix fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits
2.2 pix fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.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
14.5 mag. fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits
14.5 mag. fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 14.0 (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.LmUUyrn7T7 (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_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/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.6STK0KggMy (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_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/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.ZMxBiMqrTe (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_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.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_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits
WCS_IMAGE_NAME=wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits
WCS-calibrated image found: wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits
Checking if the catalog wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits.cat corresponding to the image wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits.cat corresponding to the image wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.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_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits
WCS catalog name: wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=2919, passed=56892
Got 56892 stars (including 53911 good ones) from the SExtractor catalog wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits.cat
util/solve_plate_with_UCAC5 got 56892 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.4'
Seting catalog search parameters based on the expected field of view 939.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013047 (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 0.010438 (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: 0.46"
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: 0.46"
Estimated accuracy of the plate solution: 0.47"
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_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits -region wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.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.T64yhxwJ6r (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_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.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_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.fits
WCS_IMAGE_NAME=wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.fits
WCS-calibrated image found: wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.fits
Checking if the catalog wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.fits.cat corresponding to the image wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.fits.cat corresponding to the image wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.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_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.fits
WCS catalog name: wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.fits.cat
SExtractor catalog parsing summary: zero_flux=2, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=2922, passed=56970
Got 56970 stars (including 53978 good ones) from the SExtractor catalog wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.fits.cat
util/solve_plate_with_UCAC5 got 56970 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.3'
Seting catalog search parameters based on the expected field of view 939.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013046 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010437 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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: 0.48"
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 958 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: 0.49"
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_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.fits -region wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.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_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/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_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/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_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.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_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-10-17_20.00sec_-14.90C_LIGHT_0429.fits
Saving fully-calibrated image wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.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_2026-03-29_CI_Peg-05-Q2b1x1_061202_TTUQ2b1x1_7819_zfwwmlCw/wcs_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430.fits
Preparing the HTML report for the field Peg-05-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out102251.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out102262.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103051.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out104503.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out105803.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107151.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107860.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out108084.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out108495.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out108964.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out109329.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out109342.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out109459.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out110726.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out111967.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112123.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112212.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112252.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112260.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112284.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112391.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out112399.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out106247.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out107962.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out109558.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out110758.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out110808.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out102246.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79028.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 65s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 102246_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
Preparing report for the candidate 102246_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
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Considering the candidate 102251_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 102251_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 21:54:13.65 +21:45:28.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 2.799 1793151977112287360 328.55754128112 +21.75841495094 13.9214 13.3579 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.799#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 102262_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 102262_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 21:59:12.76 +22:00:41.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)GAIADR2_OUTPUT=# 0.391 1782639409000237056 329.80319115781 +22.01166168950 12.7806 12.3692 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.391#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103051_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 103051_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 22:10:22.76 +25:20:04.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.21, MAG_FAINT_SEARCH_LIMIT=12.19)GAIADR2_OUTPUT=# 1.633 1891652825799000832 332.59477853599 +25.33404918652 11.2187 10.5375 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.633#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103611_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 103611_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 22:14:24.47 +22:05:40.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 104503_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 104503_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 22:18:20.74 +25:29:52.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 0.607 1879801877157896960 334.58623135734 +25.49775596153 12.3734 11.8901 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.607#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 104542_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 104542_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 22:07:43.43 +21:41:17.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 105075_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 105075_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 21:51:32.60 +19:48:10.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 105158_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 105158_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 22:26:48.74 +22:48:38.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105803_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 105803_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 21:47:08.22 +22:23:36.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 1.079 1793407235608878720 326.78442985647 +22.39361043955 12.9349 12.3834 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.079#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 106115_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 106115_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 22:15:37.01 +25:46:04.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106247_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 106247_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 21:48:31.11 +18:05:44.5 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)
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Considering the candidate 106364_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 106364_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 22:06:49.82 +25:51:42.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106963_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 106963_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 22:30:14.53 +22:26:52.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107151_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 107151_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 21:57:44.72 +23:42:12.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 0.944 1795142088862752768 329.43608818654 +23.70336434052 13.2401 12.6089 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.944#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107610_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 107610_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 21:52:20.01 +21:18:40.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107782_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 107782_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 21:47:06.24 +23:51:35.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107860_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 107860_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 22:15:57.81 +24:56:06.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 2.274 1879381928139645184 333.99116686427 +24.93574035200 13.5126 12.8495 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.274#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107957_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 107957_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 22:25:34.77 +18:27:30.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 107962_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 107962_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 21:45:40.82 +17:50:30.8 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)
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Considering the candidate 107994_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 107994_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 22:24:38.71 +24:40:22.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 108084_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 108084_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 22:14:27.74 +23:33:20.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 0.710 1878387114930747520 333.61555156809 +23.55558275621 13.8300 13.3931 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.710#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 108364_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 108364_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 22:23:20.66 +21:58:59.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 108495_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 108495_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 21:56:18.15 +22:30:38.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 4.097 1794714486214878080 329.07448043535 +22.51024557010 13.7137 13.2466 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.097#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 108530_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 108530_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 21:46:03.89 +20:01:08.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 108771_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 108771_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 22:17:59.28 +24:09:07.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 108804_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 108804_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 21:57:30.60 +23:33:01.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 108964_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 108964_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 22:11:06.60 +19:48:16.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 4.025 1778195457878626432 332.77757269425 +19.80558807942 13.9013 13.3572 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.025#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 109251_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 109251_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 22:17:55.69 +24:06:50.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 109274_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 109274_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 22:10:00.51 +22:22:42.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 109329_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 109329_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 22:21:56.27 +23:52:35.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 1.064 1878278091480800128 335.48413577292 +23.87665847602 13.5141 13.0019 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.064#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 109342_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 109342_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 21:59:02.73 +20:28:34.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 0.983 1780778245052139392 329.76151121426 +20.47643593851 13.8570 13.1619 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.983#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 109394_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 109394_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 22:24:53.58 +21:30:07.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 109395_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 109395_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 22:04:52.71 +21:16:24.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 109459_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 109459_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 21:56:10.89 +20:01:30.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.75, MAG_FAINT_SEARCH_LIMIT=14.73)GAIADR2_OUTPUT=# 3.420 1780644963626897536 329.04549273820 +20.02425077377 14.0319 13.4760 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.420#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 109558_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 109558_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 21:56:17.71 +18:19:47.2 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)
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Considering the candidate 109566_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 109566_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 21:58:52.13 +21:52:38.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 109603_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 109603_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 22:13:54.55 +22:09:52.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 109680_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 109680_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 110058_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 110058_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 21:55:16.15 +23:59:59.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 110115_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 110115_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 21:46:56.29 +21:19:14.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 110264_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 110264_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 22:04:22.58 +20:16:50.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 110726_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 110726_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 22:22:07.61 +24:33:06.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.05, MAG_FAINT_SEARCH_LIMIT=15.03)GAIADR2_OUTPUT=# 1.550 1878899762227139968 335.53173028275 +24.55223561923 13.9763 13.1205 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.550#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 110758_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 110758_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 22:14:28.59 +21:53:09.5 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)
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Considering the candidate 110808_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 110808_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 21:55:16.80 +22:12:48.3 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)
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Considering the candidate 111600_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 111600_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 22:07:53.59 +24:08:19.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 111967_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 111967_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 22:02:54.66 +25:28:55.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)GAIADR2_OUTPUT=# 4.110 1795737341267514368 330.72801175664 +25.48320033629 14.2272 13.5881 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.110#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 112123_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 112123_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 22:10:13.41 +25:43:01.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.35, MAG_FAINT_SEARCH_LIMIT=15.33)GAIADR2_OUTPUT=# 3.623 1891680691546976384 332.55699151992 +25.71716293699 14.5331 14.0233 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.623#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 112212_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 112212_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 21:57:41.25 +20:04:25.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 1.644 1780654549993867136 329.42140068504 +20.07370496970 14.4005 13.7329 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.644#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 112252_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 112252_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 22:17:11.69 +26:05:00.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)GAIADR2_OUTPUT=# 0.589 1880037928560667904 334.29864135921 +26.08356880514 14.3941 13.8004 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.589#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 112260_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 112260_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 21:44:46.75 +19:48:52.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.56, MAG_FAINT_SEARCH_LIMIT=15.54)GAIADR2_OUTPUT=# 0.820 1792453477991123968 326.19465632827 +19.81474457891 14.5673 14.0187 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.820#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 112284_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 112284_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 21:59:02.69 +23:04:11.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.68, MAG_FAINT_SEARCH_LIMIT=15.66)GAIADR2_OUTPUT=# 1.238 1794852096966895360 329.76083940489 +23.07002811775 14.7589 14.2011 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.238#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 112391_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 112391_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 21:58:14.32 +22:55:56.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.61, MAG_FAINT_SEARCH_LIMIT=15.59)GAIADR2_OUTPUT=# 1.633 1794844331665977728 329.55984471388 +22.93275618118 14.9103 14.3616 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.633#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 112399_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 112399_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks
**** FOUND 21:53:30.11 +23:04:13.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.49, MAG_FAINT_SEARCH_LIMIT=15.47)GAIADR2_OUTPUT=# 1.864 1794993212412551936 328.37492612414 +23.07058469278 14.7216 14.1256 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.864#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 70393_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430
The candidate 70393_fd_Peg-05-Q2b1x1_2026-03-29_06-11-16_20.00sec_-15.00C_LIGHT_0430 did not pass the final checks