This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt
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 27.1317 2461126.6317 13.11 03:43:14.32 +34:17:42.4
158.84672 -16.33450 galactic Per Second-epoch detections are separated by 6.3" and 2.5 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 | Gaia DR3 218200182774080000 | 03:43:15.62 +34:17:33.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
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!
TCP 2026 03 27.1317* 03 43 14.32 +34 17 42.4 13.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 218200182774080000,2461126.6317,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 218200182774080000 20260327.1317 13.11CV 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/Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:43:14.32 +34:17:42.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20_00sec_-15_00C_LIGHT_0147_fits__*pix.png resample_wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20_00sec_-10_00C_LIGHT_0075_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20_00sec_-15_00C_LIGHT_0147_fits__*pix.png resample_wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20_00sec_-10_00C_LIGHT_0074_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20_00sec_-15_00C_LIGHT_0147_fits__*pix.png resample_wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20_00sec_-10_00C_LIGHT_0075_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20_00sec_-15_00C_LIGHT_0147_fits__*pix.png resample_wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20_00sec_-10_00C_LIGHT_0074_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!
TCP 2026 03 27.1317* 03 40 09.25 +41 10 58.3 13.9 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461126.6317,13.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260327.1317 13.88CV 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/Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:40:09.25 +41:10:58.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20_00sec_-15_00C_LIGHT_0147_fits__*pix.png resample_wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20_00sec_-10_00C_LIGHT_0075_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20_00sec_-15_00C_LIGHT_0147_fits__*pix.png resample_wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20_00sec_-10_00C_LIGHT_0074_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20_00sec_-15_00C_LIGHT_0147_fits__*pix.png resample_wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20_00sec_-10_00C_LIGHT_0075_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20_00sec_-15_00C_LIGHT_0147_fits__*pix.png resample_wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20_00sec_-10_00C_LIGHT_0074_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: 2461049.67904400 09.01.2026 04:17:39.402 /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits
First image: 2461049.67904400 09.01.2026 04:17:39.402 /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits
Last image: 2461126.63200512 27.03.2026 03:09:55.242 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 9
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.51
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 15261
Objects passed selection criteria: 15203
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 11206.8
Average stars matched: 10960.8 (97.8049 %)
Memory usage VmPeak: 121472 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 26 22:14:50 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.67904400 09.01.2026 04:17:39.402 /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits
First image: 2461049.67904400 09.01.2026 04:17:39.402 /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits
Last image: 2461126.63200512 27.03.2026 03:09:55.242 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 146
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.20
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: 23 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): 106330
Objects passed selection criteria: 106079
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 2.0 2 4
Average stars detected per image: 82026
Average stars matched: 78937.8 (96.235 %)
Memory usage VmPeak: 2008556 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 26 22:16:33 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/Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits
SExtractor catalog cache: saved Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits.cat to cache
SExtractor catalog cache: saved Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.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/Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.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: 2461126.63146459
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Plate-solving the images
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits exists and is non-empty
Saving wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits to local_wcs_cache/
'wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits' -> 'local_wcs_cache/wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits'
wcs_Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits exists and is non-empty
Saving wcs_Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits to local_wcs_cache/
'wcs_Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits' -> 'local_wcs_cache/wcs_Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits'
wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits exists and is non-empty
Saving wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits to local_wcs_cache/
'wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits' -> 'local_wcs_cache/wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits'
wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits exists and is non-empty
Saving wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits to local_wcs_cache/
'wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits' -> 'local_wcs_cache/wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.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 03:16:22.482 +37:59:56.74
Second-epoch image center 03:16:31.294 +37:57:58.59
Angular distance between the image centers 0.04 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 03:16:22.482 +37:59:56.74
Second-epoch image center 03:16:32.929 +37:57:53.60
Angular distance between the image centers 0.05 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 03:16:31.294 +37:57:58.59
Second-epoch second image center 03:16:32.929 +37:57:53.60
Angular distance between the image centers 0.00555 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/Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits &> /tmp/tmp.S8B6vu1LLF
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits &> /tmp/tmp.7ePKNHv7pw
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits &> /tmp/tmp.o749EOqCy7
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits &> /tmp/tmp.PRKXbHkOwj
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits
Calibrating the magnitude scale
Found non-empty wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.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_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits and wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.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_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits and wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits.cat
Found non-empty wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits and wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits.cat
The reference image (wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits) and catalog (wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits.cat) found
'wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.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 9115 out of 19796 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.931060
a=0.000000 b=1.000000 c=22.931060
From vast_summary.log: estimated ref. image limiting mag.: -7.51
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.42
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.42
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits
2.1 pix Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits
2.6 pix fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits
2.5 pix fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits
Limiting magnitude estimates:
15.4 mag. Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits
15.4 mag. Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits
14.1 mag. fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits
14.1 mag. fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 11.3 (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.S8B6vu1LLF (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/Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits' -> 'wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits
WCS_IMAGE_NAME=wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits
WCS-calibrated image found: wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits
Checking if the catalog wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits.cat corresponding to the image wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits alredy exist and is non-empty...
Catalog wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits.cat corresponding to the image wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits
WCS catalog name: wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1744, passed=19796
Got 19796 stars (including 18022 good ones) from the SExtractor catalog wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits.cat
util/solve_plate_with_UCAC5 got 19796 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
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: 0.37"
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 955 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits -region wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.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.7ePKNHv7pw (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/Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits' -> 'wcs_Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits
WCS_IMAGE_NAME=wcs_Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits
WCS-calibrated image found: wcs_Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits
Checking if the catalog wcs_Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits.cat corresponding to the image wcs_Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits alredy exist and is non-empty...
Catalog wcs_Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits.cat corresponding to the image wcs_Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits
WCS catalog name: wcs_Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1775, passed=19606
Got 19606 stars (including 17810 good ones) from the SExtractor catalog wcs_Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits.cat
util/solve_plate_with_UCAC5 got 19606 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 959 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: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.37"
Estimated accuracy of the plate solution: 0.37"
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_Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits -region wcs_Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.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.o749EOqCy7 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits
WCS_IMAGE_NAME=wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits
WCS-calibrated image found: wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits
Checking if the catalog wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits.cat corresponding to the image wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits.cat corresponding to the image wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits
WCS catalog name: wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=508, passed=7620
Got 7620 stars (including 7106 good ones) from the SExtractor catalog wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits.cat
util/solve_plate_with_UCAC5 got 7620 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010420 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.53"
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 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.54"
Estimated accuracy of the plate solution: 0.56"
Excluding outliers - 951 stars left (next iteration limit 1046)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits -region wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.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.PRKXbHkOwj (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits
WCS_IMAGE_NAME=wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits
WCS-calibrated image found: wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits
Checking if the catalog wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits.cat corresponding to the image wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits.cat corresponding to the image wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits
WCS catalog name: wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=513, passed=7503
Got 7503 stars (including 6984 good ones) from the SExtractor catalog wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits.cat
util/solve_plate_with_UCAC5 got 7503 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010420 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 952 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: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.57"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.57"
Estimated accuracy of the plate solution: 0.60"
Excluding outliers - 949 stars left (next iteration limit 1043)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits -region wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.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_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits'
Saving fully-calibrated image wcs_Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/wcs_Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits'
Saving fully-calibrated image wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits'
Saving fully-calibrated image wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits'
Preparing the HTML report for the field Per-04-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 20824_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 20824_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 02:57:08.74 +37:53:40.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13931_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 13931_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 02:52:26.06 +36:41:30.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04193_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 04193_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 03:32:32.21 +41:26:30.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15206_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 15206_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 03:30:03.04 +35:40:17.0 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 Per-04-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/Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits
SExtractor catalog cache: saved Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits.cat to cache
SExtractor catalog cache: saved Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits
Creating symlink local_wcs_cache/wcs_Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits
Creating symlink local_wcs_cache/wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits
Creating symlink local_wcs_cache/wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.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_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits exists and is non-empty
wcs_Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits exists and is non-empty
wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits exists and is non-empty
wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.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 03:16:22.482 +37:59:56.74
Second-epoch image center 03:16:31.294 +37:57:58.59
Angular distance between the image centers 0.04 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 03:16:22.482 +37:59:56.74
Second-epoch image center 03:16:32.929 +37:57:53.60
Angular distance between the image centers 0.05 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 03:16:31.294 +37:57:58.59
Second-epoch second image center 03:16:32.929 +37:57:53.60
Angular distance between the image centers 0.00555 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/Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits &> /tmp/tmp.1CCCSSM6TO
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits &> /tmp/tmp.acO5Hxkwt7
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits &> /tmp/tmp.2QNYX3aSAm
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits &> /tmp/tmp.PHLG5atNX8
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits
Calibrating the magnitude scale
Found non-empty wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.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_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits and wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.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_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits and wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits.cat
Found non-empty wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits and wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits.cat
The reference image (wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits) and catalog (wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits.cat) found
'wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.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 9218 out of 132599 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.797170
a=0.000000 b=1.000000 c=22.797170
From vast_summary.log: estimated ref. image limiting mag.: -7.20
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.60
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.60
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 93 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits
1.9 pix Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits
2.3 pix fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits
2.2 pix fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits
Limiting magnitude estimates:
15.6 mag. Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits
15.6 mag. Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits
14.3 mag. fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits
14.3 mag. fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 13.7 (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.1CCCSSM6TO (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/Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits' -> 'wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits
WCS_IMAGE_NAME=wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits
WCS-calibrated image found: wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits
Checking if the catalog wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits.cat corresponding to the image wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits alredy exist and is non-empty...
Catalog wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits.cat corresponding to the image wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits
WCS catalog name: wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=29, blended=13812, passed=132570
Got 132570 stars (including 118539 good ones) from the SExtractor catalog wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits.cat
util/solve_plate_with_UCAC5 got 132570 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
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: 0.37"
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 955 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits -region wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.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.acO5Hxkwt7 (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/Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits' -> 'wcs_Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits
WCS_IMAGE_NAME=wcs_Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits
WCS-calibrated image found: wcs_Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits
Checking if the catalog wcs_Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits.cat corresponding to the image wcs_Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits alredy exist and is non-empty...
Catalog wcs_Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits.cat corresponding to the image wcs_Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits
WCS catalog name: wcs_Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=45, blended=14009, passed=134870
Got 134870 stars (including 120645 good ones) from the SExtractor catalog wcs_Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits.cat
util/solve_plate_with_UCAC5 got 134870 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
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: 0.39"
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 959 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits -region wcs_Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.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.2QNYX3aSAm (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits
WCS_IMAGE_NAME=wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits
WCS-calibrated image found: wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits
Checking if the catalog wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits.cat corresponding to the image wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits.cat corresponding to the image wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits
WCS catalog name: wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits.cat
SExtractor catalog parsing summary: zero_flux=2, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=3181, passed=54074
Got 54074 stars (including 50833 good ones) from the SExtractor catalog wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits.cat
util/solve_plate_with_UCAC5 got 54074 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010420 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.50"
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: 0.50"
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 956 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits -region wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.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.PHLG5atNX8 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits
WCS_IMAGE_NAME=wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits
WCS-calibrated image found: wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits
Checking if the catalog wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits.cat corresponding to the image wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits.cat corresponding to the image wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits
WCS catalog name: wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=2945, passed=55249
Got 55249 stars (including 52241 good ones) from the SExtractor catalog wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits.cat
util/solve_plate_with_UCAC5 got 55249 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010420 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
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: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.54"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
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: 0.54"
Estimated accuracy of the plate solution: 0.57"
Excluding outliers - 955 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits -region wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.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_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20.00sec_-15.00C_LIGHT_0147.fits
Saving fully-calibrated image wcs_Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/wcs_Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits
Saving fully-calibrated image wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-08_20.00sec_-10.00C_LIGHT_0074.fits
Saving fully-calibrated image wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Per-04-Q2b1x1_221239_TTUQ2b1x1_4233_iDCHwwRt/wcs_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075.fits
Preparing the HTML report for the field Per-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out143284.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out153723.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out153727.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out153729.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out153731.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out153733.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out153737.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out153749.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out153753.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out153755.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out153756.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out153761.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out153763.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out153766.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out153981.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out154253.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out154294.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out154685.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out153757.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out154647.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 16s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 153723_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 153723_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 03:01:46.73 +35:20:07.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 2.167 138790807315061888 045.44470117657 +35.33596296200 14.0802 13.4535 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.167#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 153727_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 153727_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 03:01:42.99 +35:33:47.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 3.453 138841865886210944 045.42798388904 +35.56343636551 13.8760 13.3234 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.453#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 153729_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 153729_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 03:01:47.48 +34:44:11.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.83, MAG_FAINT_SEARCH_LIMIT=14.81)GAIADR2_OUTPUT=# 1.365 137256851155168768 045.44741676644 +34.73677393657 13.7410 12.8980 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.365#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 153730_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 153730_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 02:48:56.36 +37:44:23.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 153731_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 153731_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 03:05:42.02 +41:11:28.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 0.950 239924333515177728 046.42474014593 +41.19127669847 13.4902 12.6566 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.950#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 153733_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 153733_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 03:43:52.61 +34:31:26.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 4.613 218305907689864320 055.97033264615 +34.52480190169 13.1607 12.5465 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.613#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 153737_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 153737_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 02:58:27.31 +39:53:36.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 0.789 143869245366000640 044.61353425655 +39.89348416107 13.5283 12.8133 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.789#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 153740_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 153740_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 03:09:21.60 +37:39:37.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 153749_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 153749_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 03:08:57.33 +35:02:19.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)
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Considering the candidate 153753_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 153753_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 03:11:32.07 +39:13:37.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 2.081 238719749807391616 047.88290843380 +39.22735625792 13.2209 12.4205 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.081#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 153755_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 153755_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 03:08:37.70 +35:04:06.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 0.937 138627426759137024 047.15696950202 +35.06865959062 13.2001 12.6013 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.937#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 153756_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 153756_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 02:46:55.28 +39:28:18.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 2.444 335610054476265856 041.73107347936 +39.47228320141 13.2511 12.6803 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.444#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 153757_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
Preparing report for the candidate 153757_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
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Considering the candidate 153761_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 153761_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 02:46:34.00 +37:54:53.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 0.518 141815696945332992 041.64153701995 +37.91507342841 13.2325 12.5585 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.518#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 153762_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 153762_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 02:58:43.29 +38:00:20.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 153763_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 153763_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 03:03:44.01 +39:31:17.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 2.394 142943692796244224 045.93303594934 +39.52222237461 12.9054 12.0627 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.394#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 153765_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 153765_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 03:23:21.12 +41:42:44.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 153766_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 153766_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 03:05:56.20 +40:37:47.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)
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Considering the candidate 153767_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 153767_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
Rejecting candidate due to large distance (19.5") between the two second-epoch detections
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Considering the candidate 153770_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 153770_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 02:48:24.88 +33:50:18.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 153812_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 153812_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 02:50:14.00 +34:14:00.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 153835_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 153835_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 153869_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 153869_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 153899_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 153899_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 03:03:48.06 +41:12:31.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 153910_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 153910_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 02:59:11.35 +35:09:27.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 153931_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 153931_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 02:52:46.97 +36:29:00.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 153950_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 153950_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 153959_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 153959_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 03:07:42.60 +36:35:36.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 153965_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 153965_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 153967_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 153967_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
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Considering the candidate 153981_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 153981_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 03:13:36.35 +39:09:44.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 1.673 235725058090112256 048.40138290613 +39.16276650817 13.2374 12.8564 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.673#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 153987_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 153987_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 02:49:32.34 +37:20:45.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 153997_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 153997_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 03:12:01.68 +38:32:11.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154016_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 154016_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 154034_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 154034_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 03:10:02.50 +41:42:20.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154085_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 154085_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 03:03:14.22 +41:39:07.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154089_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 154089_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 03:22:42.40 +41:56:33.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154125_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 154125_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 03:33:35.59 +39:55:37.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 154132_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 154132_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 03:00:11.33 +42:08:46.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154161_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 154161_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 02:51:30.26 +36:12:29.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154182_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 154182_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 03:35:08.30 +38:36:24.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154253_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 154253_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 02:52:49.20 +36:27:39.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)
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Considering the candidate 154270_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 154270_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 03:03:51.69 +41:13:40.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154283_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 154283_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 03:41:27.89 +36:21:57.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154294_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 154294_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 03:05:40.31 +41:29:05.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 0.726 239949072526571392 046.41771753176 +41.48492318577 13.5393 12.9117 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.726#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 154295_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 154295_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
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Considering the candidate 154296_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 154296_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 03:09:26.74 +37:16:40.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154297_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 154297_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 03:27:08.03 +41:49:52.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154323_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 154323_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 03:29:27.51 +40:34:30.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154383_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 154383_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 03:05:39.75 +36:47:03.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154395_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 154395_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 03:00:27.65 +42:03:17.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154450_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 154450_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 03:23:46.54 +40:38:37.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154451_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 154451_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
Rejecting candidate due to large distance (20.1") between the two second-epoch detections
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Considering the candidate 154453_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 154453_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 03:24:54.86 +41:58:00.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154466_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 154466_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
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Considering the candidate 154474_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 154474_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 03:07:34.23 +39:03:22.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154485_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 154485_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 03:15:15.56 +41:09:41.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154510_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 154510_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 03:27:13.06 +41:50:22.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154541_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 154541_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 154553_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 154553_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 154574_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 154574_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 154578_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 154578_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
Rejecting candidate due to large distance (21.2") between the two second-epoch detections
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Considering the candidate 154581_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 154581_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 03:05:33.35 +39:39:09.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154582_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 154582_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 02:55:54.38 +41:47:15.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154583_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 154583_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 02:52:51.59 +36:27:47.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154588_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 154588_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
Rejecting candidate due to large distance (22.3") between the two second-epoch detections
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Considering the candidate 154591_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 154591_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 154603_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 154603_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
Rejecting candidate due to large distance (19.7") between the two second-epoch detections
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Considering the candidate 154606_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 154606_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 154613_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 154613_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
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Considering the candidate 154614_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 154614_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 154617_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 154617_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 154621_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 154621_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
Rejecting candidate due to large distance (19.3") between the two second-epoch detections
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Considering the candidate 154623_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 154623_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
Rejecting candidate due to large distance (23.1") between the two second-epoch detections
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Considering the candidate 154624_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 154624_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
Rejecting candidate due to large distance (20.9") between the two second-epoch detections
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Considering the candidate 154630_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 154630_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 03:22:53.31 +38:46:06.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154638_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 154638_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
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Considering the candidate 154641_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 154641_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
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Considering the candidate 154644_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 154644_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 03:06:03.88 +40:09:42.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154646_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 154646_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 154647_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
Preparing report for the candidate 154647_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
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Considering the candidate 154663_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 154663_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
Rejecting candidate due to large distance (22.5") between the two second-epoch detections
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Considering the candidate 154672_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 154672_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
Rejecting candidate due to large distance (20.8") between the two second-epoch detections
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Considering the candidate 154673_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 154673_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 154680_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 154680_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
Rejecting candidate due to large distance (21.3") between the two second-epoch detections
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Considering the candidate 154684_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 154684_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 03:18:33.86 +37:33:31.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 154685_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 154685_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 03:18:25.85 +38:28:23.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)GAIADR2_OUTPUT=# 1.605 235527558314153856 049.60725711107 +38.47354983032 14.0276 13.3183 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.605#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 143284_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 143284_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 03:37:03.59 +33:54:00.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 0.164 220831378521194624 054.26491552379 +33.90025077794 11.6161 10.5697 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.164#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 119098_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 119098_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 03:30:03.05 +35:40:17.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 25768_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 25768_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 03:32:32.20 +41:26:30.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 80698_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 80698_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 02:57:08.73 +37:53:39.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 131804_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 131804_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks
**** FOUND 02:52:26.13 +36:41:30.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 144121_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075
The candidate 144121_fd_Per-04-Q2b1x1_2026-03-26_22-09-55_20.00sec_-10.00C_LIGHT_0075 did not pass the final checks