This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 03 27.3325 2461126.8325 12.03 19:19:23.11 +29:35:10.3
62.39670 7.52683 galactic Lyr Second-epoch detections are separated by 1.8" and 9.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 2038416737406013184 | 19:19:22.59 +29:35:12.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 2038416737406013184,2461126.8325,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 2038416737406013184 20260327.3325 12.03CV 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/Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:19:23.11 +29:35:10.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20_00sec_-15_00C_LIGHT_0401_fits__*pix.png resample_wcs_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20_00sec_-14_90C_LIGHT_0327_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20_00sec_-15_00C_LIGHT_0401_fits__*pix.png resample_wcs_fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20_00sec_-14_90C_LIGHT_0325_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20_00sec_-15_00C_LIGHT_0401_fits__*pix.png resample_wcs_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20_00sec_-14_90C_LIGHT_0327_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20_00sec_-15_00C_LIGHT_0401_fits__*pix.png resample_wcs_fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20_00sec_-14_90C_LIGHT_0325_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.3325 2461126.8325 12.62 18:51:53.43 +28:57:15.8
59.18923 12.66263 galactic Lyr Second-epoch detections are separated by 1.2" and 9.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J282.9695+28.9591 | 18:51:53.01 +28:57:12.5 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J282.9695+28.9591,2461126.8325,12.62,0.05,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
ATO J282.9695+28.9591 20260327.3325 12.62CV 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/Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:51:53.43 +28:57:15.8 ;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_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20_00sec_-15_00C_LIGHT_0401_fits__*pix.png resample_wcs_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20_00sec_-14_90C_LIGHT_0327_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20_00sec_-15_00C_LIGHT_0401_fits__*pix.png resample_wcs_fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20_00sec_-14_90C_LIGHT_0325_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20_00sec_-15_00C_LIGHT_0401_fits__*pix.png resample_wcs_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20_00sec_-14_90C_LIGHT_0327_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20_00sec_-15_00C_LIGHT_0401_fits__*pix.png resample_wcs_fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20_00sec_-14_90C_LIGHT_0325_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: 2461121.99435186 22.03.2026 11:51:42.001 /data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits
First image: 2461121.99435186 22.03.2026 11:51:42.001 /data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits
Last image: 2461126.83426543 27.03.2026 08:01:10.533 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.10
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 5 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 17520
Objects passed selection criteria: 17445
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 12776.5
Average stars matched: 12500.5 (97.8398 %)
Memory usage VmPeak: 124108 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 Fri Mar 27 03:03:09 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: 2461121.99435186 22.03.2026 11:51:42.001 /data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits
First image: 2461121.99435186 22.03.2026 11:51:42.001 /data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits
Last image: 2461126.83426543 27.03.2026 08:01:10.533 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 33
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.77
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: 30 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): 151621
Objects passed selection criteria: 151218
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 106264
Average stars matched: 102962 (96.8931 %)
Memory usage VmPeak: 2710400 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 Fri Mar 27 03:06:07 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/Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits
SExtractor catalog cache: saved Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits.cat to cache
SExtractor catalog cache: saved Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.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/Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461126.83065956
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Plate-solving the images
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits exists and is non-empty
Saving wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits to local_wcs_cache/
'wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits' -> 'local_wcs_cache/wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits'
wcs_Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits exists and is non-empty
Saving wcs_Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits to local_wcs_cache/
'wcs_Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits' -> 'local_wcs_cache/wcs_Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits'
wcs_fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits exists and is non-empty
Saving wcs_fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits to local_wcs_cache/
'wcs_fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits' -> 'local_wcs_cache/wcs_fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits'
wcs_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits exists and is non-empty
Saving wcs_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits to local_wcs_cache/
'wcs_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits' -> 'local_wcs_cache/wcs_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.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 19:00:00.980 +30:00:09.31
Second-epoch image center 18:59:56.969 +29:58:00.14
Angular distance between the image centers 0.04 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 19:00:00.980 +30:00:09.31
Second-epoch image center 19:00:00.303 +29:58:34.77
Angular distance between the image centers 0.03 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 18:59:56.969 +29:58:00.14
Second-epoch second image center 19:00:00.303 +29:58:34.77
Angular distance between the image centers 0.01541 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/Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits &> /tmp/tmp.Jq9khwMQjN
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits &> /tmp/tmp.7R6gHZgRoY
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits &> /tmp/tmp.hzinjzsul3
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits &> /tmp/tmp.s45AnHj6HO
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits
Calibrating the magnitude scale
Found non-empty wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.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_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits and wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.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_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits and wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits.cat
Found non-empty wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits and wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits.cat
The reference image (wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits) and catalog (wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits.cat) found
'wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.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 16943 out of 24593 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.970305
a=0.000000 b=1.000000 c=22.970305
From vast_summary.log: estimated ref. image limiting mag.: -8.10
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.87
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.87
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits
2.1 pix Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits
4.7 pix fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits
2.9 pix fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits
Limiting magnitude estimates:
14.9 mag. Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits
14.8 mag. Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits
13.2 mag. fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits
13.6 mag. fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits
All-image limiting magnitude estimate: 13.2 (SNR ) 10.8 (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.Jq9khwMQjN (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/Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.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_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits' -> 'wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits
WCS_IMAGE_NAME=wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits
WCS-calibrated image found: wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits
Checking if the catalog wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits.cat corresponding to the image wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits alredy exist and is non-empty...
Catalog wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits.cat corresponding to the image wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits
WCS catalog name: wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2529, passed=24593
Got 24593 stars (including 22035 good ones) from the SExtractor catalog wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits.cat
util/solve_plate_with_UCAC5 got 24593 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.48"
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 957 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits -region wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.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.7R6gHZgRoY (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/Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.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_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits' -> 'wcs_Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits
WCS_IMAGE_NAME=wcs_Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits
WCS-calibrated image found: wcs_Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits
Checking if the catalog wcs_Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits.cat corresponding to the image wcs_Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits alredy exist and is non-empty...
Catalog wcs_Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits.cat corresponding to the image wcs_Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits
WCS catalog name: wcs_Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2382, passed=23338
Got 23338 stars (including 20928 good ones) from the SExtractor catalog wcs_Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits.cat
util/solve_plate_with_UCAC5 got 23338 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.50"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.50"
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits -region wcs_Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.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.hzinjzsul3 (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_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.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_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits
WCS_IMAGE_NAME=wcs_fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits
WCS-calibrated image found: wcs_fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits
Checking if the catalog wcs_fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits.cat corresponding to the image wcs_fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits.cat corresponding to the image wcs_fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits
WCS catalog name: wcs_fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=211, passed=6707
Got 6707 stars (including 6495 good ones) from the SExtractor catalog wcs_fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits.cat
util/solve_plate_with_UCAC5 got 6707 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.0'
Seting catalog search parameters based on the expected field of view 939.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013042 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010433 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.79"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.80"
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: 0.81"
Estimated accuracy of the plate solution: 0.90"
Excluding outliers - 947 stars left (next iteration limit 1040)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits -region wcs_fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.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.s45AnHj6HO (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_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.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_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits
WCS_IMAGE_NAME=wcs_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits
WCS-calibrated image found: wcs_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits
Checking if the catalog wcs_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits.cat corresponding to the image wcs_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits.cat corresponding to the image wcs_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits
WCS catalog name: wcs_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=368, passed=8894
Got 8894 stars (including 8521 good ones) from the SExtractor catalog wcs_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits.cat
util/solve_plate_with_UCAC5 got 8894 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.8'
Seting catalog search parameters based on the expected field of view 938.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013039 (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 0.010431 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.70"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.71"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.71"
Estimated accuracy of the plate solution: 0.75"
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_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits -region wcs_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.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_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits'
Saving fully-calibrated image wcs_Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/wcs_Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits'
Saving fully-calibrated image wcs_fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/wcs_fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits'
Saving fully-calibrated image wcs_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/wcs_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits'
Preparing the HTML report for the field Lyr-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Lyr-03-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/Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits
SExtractor catalog cache: saved Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits.cat to cache
SExtractor catalog cache: saved Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits
Creating symlink local_wcs_cache/wcs_Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits
Creating symlink local_wcs_cache/wcs_fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits
Creating symlink local_wcs_cache/wcs_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.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_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits exists and is non-empty
wcs_Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits exists and is non-empty
wcs_fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits exists and is non-empty
wcs_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.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 19:00:00.980 +30:00:09.31
Second-epoch image center 18:59:56.969 +29:58:00.14
Angular distance between the image centers 0.04 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 19:00:00.980 +30:00:09.31
Second-epoch image center 19:00:00.303 +29:58:34.77
Angular distance between the image centers 0.03 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 18:59:56.969 +29:58:00.14
Second-epoch second image center 19:00:00.303 +29:58:34.77
Angular distance between the image centers 0.01541 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/Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits &> /tmp/tmp.zK1OpVonIK
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits &> /tmp/tmp.bsXWIrvEQf
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits &> /tmp/tmp.pcAWOx2tlf
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits &> /tmp/tmp.cRzYHF7cNQ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits
Calibrating the magnitude scale
Found non-empty wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.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_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits and wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.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_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits and wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits.cat
Found non-empty wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits and wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits.cat
The reference image (wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits) and catalog (wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits.cat) found
'wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.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 19649 out of 206271 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.787801
a=0.000000 b=1.000000 c=22.787801
From vast_summary.log: estimated ref. image limiting mag.: -7.77
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.02
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.02
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 21 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits
2.0 pix Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits
4.7 pix fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits
2.8 pix fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits
Limiting magnitude estimates:
15.0 mag. Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits
15.0 mag. Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits
13.2 mag. fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits
13.7 mag. fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits
All-image limiting magnitude estimate: 13.2 (SNR ) 12.6 (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.zK1OpVonIK (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/Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.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_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits' -> 'wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits
WCS_IMAGE_NAME=wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits
WCS-calibrated image found: wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits
Checking if the catalog wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits.cat corresponding to the image wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits alredy exist and is non-empty...
Catalog wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits.cat corresponding to the image wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits
WCS catalog name: wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=1, no_mag_err=0, low_SNR=45, blended=27248, passed=206225
Got 206225 stars (including 178636 good ones) from the SExtractor catalog wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits.cat
util/solve_plate_with_UCAC5 got 206225 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.47"
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 954 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_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits -region wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.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.bsXWIrvEQf (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/Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.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_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits' -> 'wcs_Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits
WCS_IMAGE_NAME=wcs_Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits
WCS-calibrated image found: wcs_Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits
Checking if the catalog wcs_Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits.cat corresponding to the image wcs_Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits alredy exist and is non-empty...
Catalog wcs_Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits.cat corresponding to the image wcs_Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits
WCS catalog name: wcs_Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=38, blended=25024, passed=198155
Got 198155 stars (including 172809 good ones) from the SExtractor catalog wcs_Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits.cat
util/solve_plate_with_UCAC5 got 198155 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.52"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.50"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.50"
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 950 stars left (next iteration limit 1046)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits -region wcs_Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.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.pcAWOx2tlf (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_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.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_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits
WCS_IMAGE_NAME=wcs_fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits
WCS-calibrated image found: wcs_fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits
Checking if the catalog wcs_fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits.cat corresponding to the image wcs_fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits.cat corresponding to the image wcs_fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits
WCS catalog name: wcs_fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=2582, passed=37978
Got 37978 stars (including 35373 good ones) from the SExtractor catalog wcs_fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits.cat
util/solve_plate_with_UCAC5 got 37978 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.0'
Seting catalog search parameters based on the expected field of view 939.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013042 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010433 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.80"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.81"
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 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.81"
Estimated accuracy of the plate solution: 0.91"
Excluding outliers - 946 stars left (next iteration limit 1040)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits -region wcs_fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.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.cRzYHF7cNQ (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_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.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_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits
WCS_IMAGE_NAME=wcs_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits
WCS-calibrated image found: wcs_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits
Checking if the catalog wcs_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits.cat corresponding to the image wcs_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits.cat corresponding to the image wcs_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits
WCS catalog name: wcs_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=3798, passed=65836
Got 65836 stars (including 61962 good ones) from the SExtractor catalog wcs_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits.cat
util/solve_plate_with_UCAC5 got 65836 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.8'
Seting catalog search parameters based on the expected field of view 938.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013039 (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 0.010431 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.73"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.71"
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: 0.71"
Estimated accuracy of the plate solution: 0.75"
Excluding outliers - 948 stars left (next iteration limit 1042)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits -region wcs_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.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_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.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_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/wcs_Lyr-03-Q2b1x1_2026-03-22_06-51-42_20.00sec_-15.00C_LIGHT_0401.fits
Saving fully-calibrated image wcs_Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.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_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/wcs_Lyr-03-Q2b1x1_2026-03-22_06-52-35_20.00sec_-14.90C_LIGHT_0402.fits
Saving fully-calibrated image wcs_fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.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_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/wcs_fd_Lyr-03-Q2b1x1_2026-03-27_02-55-58_20.00sec_-14.90C_LIGHT_0325.fits
Saving fully-calibrated image wcs_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.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_2026-03-27_CI_Lyr-03-Q2b1x1_030148_TTUQ2b1x1_18028_7uNIqUdJ/wcs_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327.fits
Preparing the HTML report for the field Lyr-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out228351.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out228353.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out228354.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out228356.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out228361.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out228362.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out228368.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out228371.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out228377.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out228378.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out228383.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out228694.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out228375.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out86890.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 15s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 228351_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327
The candidate 228351_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327 did not pass the final checks
**** FOUND 19:16:36.66 +27:38:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 1.110 2036451768374467072 289.15257247263 +27.64870685114 12.2001 11.7594 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.110#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 228353_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327
The candidate 228353_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327 did not pass the final checks
**** FOUND 18:33:43.41 +29:06:44.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)GAIADR2_OUTPUT=# 2.605 4587366887105977856 278.43162387835 +29.11275338371 12.8436 12.3586 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.605#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 228354_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327
The candidate 228354_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327 did not pass the final checks
**** FOUND 19:01:27.68 +32:18:56.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 1.239 2043620240588458624 285.36556098923 +32.31597981076 12.1196 11.2119 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.239#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 228356_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327
The candidate 228356_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327 did not pass the final checks
**** FOUND 19:03:51.52 +32:13:35.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 0.580 2043560905623280512 285.96485409975 +32.22647316560 12.4987 12.0148 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.580#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 228361_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327
The candidate 228361_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327 did not pass the final checks
**** FOUND 18:56:05.14 +33:35:51.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 4.062 2092028786923294592 284.02109808591 +33.59640337737 12.2092 11.7778 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.062#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 228362_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327
The candidate 228362_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327 did not pass the final checks
**** FOUND 19:23:46.52 +32:28:09.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 3.465 2045887059918996608 290.94392934613 +32.46840203472 12.0633 11.2560 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.465#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 228368_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327
The candidate 228368_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327 did not pass the final checks
**** FOUND 18:30:04.35 +31:15:23.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.46, MAG_FAINT_SEARCH_LIMIT=13.44)GAIADR2_OUTPUT=# 0.893 4588966058049398016 277.51841465130 +31.25642981631 11.9444 11.1102 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.893#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 228371_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327
The candidate 228371_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327 did not pass the final checks
**** FOUND 19:21:21.36 +30:57:24.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 5.557 2039716424552858368 290.33832470567 +30.95815301632 12.9489 12.5045 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.557#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 228375_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327
Preparing report for the candidate 228375_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327
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Considering the candidate 228377_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327
The candidate 228377_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327 did not pass the final checks
**** FOUND 19:26:28.06 +30:16:35.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 5.487 2038707386442359808 291.61572685400 +30.27754250117 11.7633 11.0390 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.487#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 228378_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327
The candidate 228378_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327 did not pass the final checks
**** FOUND 19:24:48.69 +29:55:10.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 1.990 2038671957230470656 291.20228445564 +29.91981953356 12.1913 11.9978 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.990#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 228383_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327
The candidate 228383_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327 did not pass the final checks
**** FOUND 19:28:02.17 +30:22:50.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.87, MAG_FAINT_SEARCH_LIMIT=12.85)GAIADR2_OUTPUT=# 3.039 2038703636909258112 292.00912046494 +30.38156362693 11.6192 10.8936 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.039#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 228387_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327
The candidate 228387_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327 did not pass the final checks
**** FOUND 18:29:06.44 +33:54:57.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 228694_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327
The candidate 228694_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327 did not pass the final checks
**** FOUND 19:00:12.22 +32:08:48.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 3.798 2043600384957154048 285.05209254747 +32.14654015120 11.9251 11.3302 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.798#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 86890_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327
Preparing report for the candidate 86890_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327
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Considering the candidate 107613_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327
The candidate 107613_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327 did not pass the final checks
**** FOUND 19:05:47.14 +29:55:18.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 178284_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327
The candidate 178284_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327 did not pass the final checks
**** FOUND 19:01:48.40 +33:37:17.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 38274_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327
The candidate 38274_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327 did not pass the final checks
**** FOUND 19:11:31.05 +26:44:08.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 62736_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327
The candidate 62736_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327 did not pass the final checks
**** FOUND 19:15:59.49 +27:55:35.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 185950_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327
The candidate 185950_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327 did not pass the final checks
**** FOUND 19:23:34.21 +33:13:23.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 181428_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327
The candidate 181428_fd_Lyr-03-Q2b1x1_2026-03-27_03-01-10_20.00sec_-14.90C_LIGHT_0327 did not pass the final checks