This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 26.1174* 03 05 42.83 +36 47 15.0 13.7 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
target,2461125.6174,13.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260326.1174 13.74CV 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_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:05:42.83 +36:47:15.0 ;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_2026-03-25_21-49-16_20_00sec_-10_00C_LIGHT_0301_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_2026-03-25_21-48-27_20_00sec_-10_00C_LIGHT_0300_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_2026-03-25_21-49-16_20_00sec_-10_00C_LIGHT_0301_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_2026-03-25_21-48-27_20_00sec_-10_00C_LIGHT_0300_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 26.1174* 03 37 26.21 +41 09 43.2 13.8 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,2461125.6174,13.81,0.05,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 20260326.1174 13.81CV 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_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:37:26.21 +41:09:43.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Per-04-Q2b1x1_2026-01-08_22-17-39_20_00sec_-15_00C_LIGHT_0147_fits__*pix.png resample_wcs_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20_00sec_-10_00C_LIGHT_0301_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_2026-03-25_21-48-27_20_00sec_-10_00C_LIGHT_0300_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_2026-03-25_21-49-16_20_00sec_-10_00C_LIGHT_0301_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_2026-03-25_21-48-27_20_00sec_-10_00C_LIGHT_0300_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 26.1174* 02 57 08.74 +37 53 39.8 11.7 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
LS Per,2461125.6174,11.66,0.05,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
LS Per 20260326.1174 11.66CV 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/reference_imgs/Per-04-Q2b1x1_2026-01-08_22-18-45_20.00sec_-15.00C_LIGHT_0148.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 02:57:08.74 +37:53:39.8 ;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_2026-03-25_21-49-16_20_00sec_-10_00C_LIGHT_0301_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_2026-03-25_21-48-27_20_00sec_-10_00C_LIGHT_0300_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_2026-03-25_21-49-16_20_00sec_-10_00C_LIGHT_0301_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_2026-03-25_21-48-27_20_00sec_-10_00C_LIGHT_0300_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: 2461125.61766580 26.03.2026 02:49:16.325 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 10
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): 15314
Objects passed selection criteria: 15266
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 11998.2
Average stars matched: 11735 (97.8059 %)
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 Wed Mar 25 22:04:25 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: 2461125.61766580 26.03.2026 02:49:16.325 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 155
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: 77 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): 106809
Objects passed selection criteria: 106579
Measurements per detected object (mean, median, min, max): 3.1 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 3.0 2 4
Average stars detected per image: 87472.8
Average stars matched: 84268.2 (96.3366 %)
Memory usage VmPeak: 1943020 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 Wed Mar 25 22:06:59 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/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_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.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_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461125.61710050
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_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_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits exists and is non-empty
Saving wcs_fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits to local_wcs_cache/
'wcs_fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits' -> 'local_wcs_cache/wcs_fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits'
wcs_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.fits exists and is non-empty
Saving wcs_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.fits to local_wcs_cache/
'wcs_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.fits' -> 'local_wcs_cache/wcs_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.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 03:16:43.493 +38:03:48.41
Angular distance between the image centers 0.09 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 03:16:44.676 +38:03:30.88
Angular distance between the image centers 0.09 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 03:16:43.493 +38:03:48.41
Second-epoch second image center 03:16:44.676 +38:03:30.88
Angular distance between the image centers 0.00623 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.p9extr0IvS
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.msTdqWNY30
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_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits &> /tmp/tmp.NDKSVQc8zh
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.fits &> /tmp/tmp.jpNUdYHcj1
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.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 5 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
2.5 pix fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits
2.5 pix fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.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
14.4 mag. fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits
14.4 mag. fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 11.5 (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.p9extr0IvS (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_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/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.msTdqWNY30 (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_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/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.NDKSVQc8zh (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_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.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_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits
WCS_IMAGE_NAME=wcs_fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits
WCS-calibrated image found: wcs_fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits
Checking if the catalog wcs_fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits.cat corresponding to the image wcs_fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits.cat corresponding to the image wcs_fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.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_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits
WCS catalog name: wcs_fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=677, passed=9488
Got 9488 stars (including 8799 good ones) from the SExtractor catalog wcs_fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits.cat
util/solve_plate_with_UCAC5 got 9488 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (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: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.59"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
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: 0.60"
Estimated accuracy of the plate solution: 0.67"
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_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits -region wcs_fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.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.jpNUdYHcj1 (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_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.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_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.fits
WCS_IMAGE_NAME=wcs_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.fits
WCS-calibrated image found: wcs_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.fits
Checking if the catalog wcs_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.fits.cat corresponding to the image wcs_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.fits.cat corresponding to the image wcs_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.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_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.fits
WCS catalog name: wcs_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=631, passed=9497
Got 9497 stars (including 8856 good ones) from the SExtractor catalog wcs_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.fits.cat
util/solve_plate_with_UCAC5 got 9497 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (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 953 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: 0.57"
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 953 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: 0.61"
Excluding outliers - 950 stars left (next iteration limit 1045)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.fits -region wcs_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.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_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/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_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/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_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/wcs_fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits'
Saving fully-calibrated image wcs_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/wcs_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.fits'
Preparing the HTML report for the field Per-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20921.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 1s
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 20921_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 20921_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:27:26.69 +39:12:27.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.80, MAG_FAINT_SEARCH_LIMIT=11.78)GAIADR2_OUTPUT=# 0.353 235198392020615040 051.86113688895 +39.20744692513 10.7590 10.4692 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.353#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20987_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 20987_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 02:59:33.04 +41:00:51.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13931_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 13931_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 02:52:26.12 +36:41:31.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 04193_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 04193_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:32:32.23 +41:26:30.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 15206_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 15206_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:30:03.04 +35:40:16.8 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
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_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.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_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.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_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits
Creating symlink local_wcs_cache/wcs_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.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_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits exists and is non-empty
wcs_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.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 03:16:43.493 +38:03:48.41
Angular distance between the image centers 0.09 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 03:16:44.676 +38:03:30.88
Angular distance between the image centers 0.09 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 03:16:43.493 +38:03:48.41
Second-epoch second image center 03:16:44.676 +38:03:30.88
Angular distance between the image centers 0.00623 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.32rgBlFYVU
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.zQMgI7ladB
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_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits &> /tmp/tmp.a5Apmkw4a2
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.fits &> /tmp/tmp.KWpGaScvM3
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.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 110 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
2.2 pix fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits
2.3 pix fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.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
14.6 mag. fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits
14.6 mag. fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 14.0 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.32rgBlFYVU (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_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/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.zQMgI7ladB (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_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/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.a5Apmkw4a2 (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_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.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_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits
WCS_IMAGE_NAME=wcs_fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits
WCS-calibrated image found: wcs_fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits
Checking if the catalog wcs_fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits.cat corresponding to the image wcs_fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits.cat corresponding to the image wcs_fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.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_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits
WCS catalog name: wcs_fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=4210, passed=66774
Got 66774 stars (including 62473 good ones) from the SExtractor catalog wcs_fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits.cat
util/solve_plate_with_UCAC5 got 66774 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (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 957 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: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.55"
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 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.56"
Estimated accuracy of the plate solution: 0.60"
Excluding outliers - 955 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits -region wcs_fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.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.KWpGaScvM3 (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_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.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_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.fits
WCS_IMAGE_NAME=wcs_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.fits
WCS-calibrated image found: wcs_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.fits
Checking if the catalog wcs_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.fits.cat corresponding to the image wcs_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.fits.cat corresponding to the image wcs_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.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_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.fits
WCS catalog name: wcs_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=21, blended=4210, passed=66229
Got 66229 stars (including 61946 good ones) from the SExtractor catalog wcs_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.fits.cat
util/solve_plate_with_UCAC5 got 66229 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.6'
Seting catalog search parameters based on the expected field of view 937.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013022 (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 0.010418 (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 957 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: 0.53"
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 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.53"
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 955 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.fits -region wcs_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.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_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/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_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/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_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.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_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/wcs_fd_Per-04-Q2b1x1_2026-03-25_21-48-27_20.00sec_-10.00C_LIGHT_0300.fits
Saving fully-calibrated image wcs_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.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_2026-03-25_CI_Per-04-Q2b1x1_220106_TTUQ2b1x1_15050_1Q1Ls8xs/wcs_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301.fits
Preparing the HTML report for the field Per-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out153724.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out153728.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out153731.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out153735.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out153738.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out153742.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out153749.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out153750.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out153753.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out153761.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out154026.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out154040.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out154085.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out154090.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out154216.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out154239.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out154301.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out154378.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out154612.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out154660.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out154675.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out154707.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out154718.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out154736.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out154737.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out154816.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out154293.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out154394.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out154473.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out154474.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out80698.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 17s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 153718_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 153718_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:04:11.38 +38:39:48.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 153723_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 153723_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:23:32.54 +41:43:35.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 153724_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 153724_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 02:56:25.81 +35:52:05.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 0.729 140414953491281280 044.10731283066 +35.86824784386 13.8628 13.3025 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.729#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 153728_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 153728_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:20:41.61 +38:52:53.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.09, MAG_FAINT_SEARCH_LIMIT=15.07)GAIADR2_OUTPUT=# 1.404 235521064323435904 050.17287627260 +38.88150865818 14.0322 13.3408 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.404#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 153729_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 153729_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 02:52:39.01 +37:50:06.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 153731_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 153731_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:17:12.00 +38:37:07.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 2.177 235546250011817856 049.29925034199 +38.61857172036 14.2356 13.5879 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.177#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 153735_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 153735_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:28:38.51 +41:31:58.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 1.665 237687411468191360 052.16018201097 +41.53324712115 13.8678 13.3094 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.665#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 153738_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 153738_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:13:55.80 +41:09:46.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.75, MAG_FAINT_SEARCH_LIMIT=14.73)GAIADR2_OUTPUT=# 1.004 239537202343084288 048.48225603316 +41.16279012934 13.6327 12.7933 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.004#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 153740_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 153740_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 02:48:56.34 +37:44:24.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 153742_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 153742_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:01:24.62 +36:24:05.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 1.498 141907269944692352 045.35300859005 +36.40162536295 13.8775 13.1379 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.498#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 153746_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 153746_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:09:21.55 +37:39:38.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 153749_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 153749_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:13:30.79 +38:54:01.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 1.945 235706091514605696 048.37765151746 +38.90073697696 13.2532 12.2028 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.945#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 153750_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 153750_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 02:46:29.31 +37:45:25.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 1.094 141717050136473216 041.62175698279 +37.75691250037 13.8086 13.3923 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.094#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 153753_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 153753_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:09:23.46 +42:00:04.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 153759_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 153759_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:23:21.16 +41:42:45.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 153761_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 153761_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:05:02.54 +37:05:55.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 1.893 142049141304410368 046.26056024939 +37.09935893484 12.7631 12.0629 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.893#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 153837_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 153837_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
Rejecting candidate due to large distance (21.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 153839_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 153839_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 02:59:32.96 +41:00:50.1 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 153912_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 153912_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:24:41.77 +40:46:16.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 153921_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 153921_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 153949_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 153949_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 02:59:11.37 +35:09:28.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 153978_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 153978_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:03:48.08 +41:12:32.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 153989_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 153989_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
Rejecting candidate due to large distance (21.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154026_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154026_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:07:42.64 +36:35:37.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 0.508 138960647501592448 046.92749939887 +36.59376596309 12.5683 11.7670 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.508#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154028_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154028_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 02:52:46.94 +36:28:60.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154040_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154040_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:11:23.11 +38:08:41.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 0.884 139580183647645184 047.84598540375 +38.14467402622 12.8776 12.1255 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.884#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154067_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154067_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 02:49:32.37 +37:20:45.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154085_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154085_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 02:51:30.22 +36:12:29.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 1.693 140590089374572672 042.87591827094 +36.20783515898 13.2568 12.4561 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.693#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154086_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154086_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:12:01.72 +38:32:11.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154090_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154090_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:10:02.53 +41:42:20.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154092_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154092_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:34:25.95 +41:56:14.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154097_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154097_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:22:42.39 +41:56:32.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154113_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154113_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:41:27.95 +36:21:58.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154148_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154148_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
Rejecting candidate due to large distance (21.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154172_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154172_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:33:35.61 +39:55:38.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154211_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154211_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:28:26.11 +40:11:26.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154215_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154215_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 02:46:55.77 +35:33:12.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154216_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154216_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:04:50.93 +35:00:39.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 1.097 138571832702413184 046.21186382914 +35.01097650622 13.2446 12.4880 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.097#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154224_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154224_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:00:11.31 +42:08:46.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154238_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154238_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:00:27.57 +42:03:17.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154239_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154239_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 02:49:48.72 +35:31:53.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 1.450 140532536812789248 042.45300944759 +35.53181927261 13.4713 12.9488 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.450#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154259_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154259_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:03:51.70 +41:13:40.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154276_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154276_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:29:27.58 +40:34:30.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154293_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154293_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:40:56.69 +41:16:41.9 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154301_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154301_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:22:20.29 +40:17:43.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 0.487 236299346758323712 050.58439701271 +40.29543948541 13.6058 13.1564 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.487#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154302_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154302_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154304_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154304_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:07:34.26 +39:03:22.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154315_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154315_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:44:29.62 +36:26:08.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154332_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154332_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 02:47:40.03 +37:25:25.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154343_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154343_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 02:59:40.92 +33:50:25.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154357_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154357_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 02:57:17.72 +33:57:04.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154364_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154364_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:23:46.43 +40:38:38.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154368_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154368_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:24:54.96 +41:58:00.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154378_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154378_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 02:52:51.45 +36:27:47.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 1.730 140693787064665088 043.21494550206 +36.46322626682 13.7038 13.1862 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.730#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154383_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154383_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 02:55:54.61 +41:47:17.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154394_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154394_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:29:33.42 +41:51:22.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154399_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154399_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:15:15.73 +41:09:41.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154404_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154404_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154407_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154407_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 02:49:50.89 +35:51:35.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154408_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154408_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 02:55:42.20 +35:33:02.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154438_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154438_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:03:57.81 +42:12:55.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154441_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154441_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:05:33.35 +39:39:09.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154446_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154446_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:09:26.78 +37:16:41.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154462_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154462_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:25:48.99 +38:13:41.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154473_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
Preparing report for the candidate 154473_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154474_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
Preparing report for the candidate 154474_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154479_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154479_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
Rejecting candidate due to large distance (22.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154483_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154483_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:27:13.27 +41:50:22.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154532_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154532_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:11:25.13 +38:02:20.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154612_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154612_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:01:45.14 +38:31:03.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 1.992 142782137603277440 045.43866838275 +38.51789435493 13.9540 13.4127 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.992#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154626_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154626_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:24:39.80 +39:36:53.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154660_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154660_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:00:02.20 +39:25:20.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)GAIADR2_OUTPUT=# 1.941 143587323712438528 045.00848878819 +39.42240656039 14.0377 13.3422 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.941#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154671_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154671_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
Rejecting candidate due to large distance (21.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154672_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154672_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
Rejecting candidate due to large distance (22.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154675_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154675_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:09:04.60 +37:24:21.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 1.614 139444771918711552 047.26890272624 +37.40639621235 13.8629 13.1901 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.614#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154681_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154681_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:12:26.96 +41:29:19.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154694_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154694_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154704_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154704_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
Rejecting candidate due to large distance (22.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154707_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154707_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:26:49.54 +37:55:05.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 1.354 234835106506400128 051.70607908261 +37.91845993314 13.8808 13.4718 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.354#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154718_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154718_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:08:41.10 +35:28:00.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 2.750 138655395586129024 047.17070447072 +35.46737149095 14.2127 13.6428 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.750#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154726_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154726_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154735_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154735_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
Rejecting candidate due to large distance (22.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154736_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154736_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:37:57.23 +34:56:42.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 2.274 221318466469246720 054.48772556940 +34.94544539310 13.3534 12.4071 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.274#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154737_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154737_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:06:04.01 +40:09:44.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.05, MAG_FAINT_SEARCH_LIMIT=15.03)GAIADR2_OUTPUT=# 2.793 239064755940102912 046.51593148103 +40.16191729970 14.1731 13.8186 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.793#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154753_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154753_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:27:20.52 +40:08:05.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154772_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154772_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
Rejecting candidate due to large distance (22.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154773_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154773_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154780_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154780_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154787_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154787_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154790_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154790_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154798_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154798_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154807_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154807_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154812_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154812_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
Rejecting candidate due to large distance (22.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154813_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154813_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
Rejecting candidate due to large distance (22.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154816_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154816_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:04:52.57 +41:12:30.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 1.343 239916362055696384 046.21876495112 +41.20819049007 14.0531 13.3474 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.343#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154817_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154817_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:22:53.38 +38:46:07.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154833_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154833_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
Rejecting candidate due to large distance (22.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154840_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154840_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154851_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154851_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
Rejecting candidate due to large distance (21.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154861_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154861_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:02:50.11 +39:49:36.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154865_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154865_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
Rejecting candidate due to large distance (22.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154871_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154871_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154876_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154876_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
Rejecting candidate due to large distance (21.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154892_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154892_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
Rejecting candidate due to large distance (20.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 154895_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 154895_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:18:28.72 +38:21:16.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 119098_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 119098_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:30:03.06 +35:40:16.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25768_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 25768_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 03:32:32.22 +41:26:30.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 80698_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
Preparing report for the candidate 80698_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 131804_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 131804_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks
**** FOUND 02:52:26.16 +36:41:30.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 144121_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301
The candidate 144121_fd_Per-04-Q2b1x1_2026-03-25_21-49-16_20.00sec_-10.00C_LIGHT_0301 did not pass the final checks