This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 26.2910* 15 53 33.71 +11 51 08.8 13.1 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461125.7910,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260326.2910 13.13CV 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/Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:53:33.71 +11:51:08.8 ;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_Ser-02-Q2b1x1_2026-02-22_05-09-44_20_00sec_-15_00C_LIGHT_0543_fits__*pix.png resample_wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20_00sec_-10_00C_LIGHT_0541_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20_00sec_-15_00C_LIGHT_0543_fits__*pix.png resample_wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20_00sec_-10_00C_LIGHT_0540_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20_00sec_-15_00C_LIGHT_0543_fits__*pix.png resample_wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20_00sec_-10_00C_LIGHT_0541_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20_00sec_-15_00C_LIGHT_0543_fits__*pix.png resample_wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20_00sec_-10_00C_LIGHT_0540_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 26.2910* 16 16 05.84 +14 25 49.6 12.1 U Her 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
1SWASP J161605.83+142549.4,2461125.7910,12.14,0.05,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
1SWASP J161605.83+142549.4 20260326.2910 12.14CV 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/Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:16:05.84 +14:25:49.6 ;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_Ser-02-Q2b1x1_2026-02-22_05-09-44_20_00sec_-15_00C_LIGHT_0543_fits__*pix.png resample_wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20_00sec_-10_00C_LIGHT_0541_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20_00sec_-15_00C_LIGHT_0543_fits__*pix.png resample_wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20_00sec_-10_00C_LIGHT_0540_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20_00sec_-15_00C_LIGHT_0543_fits__*pix.png resample_wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20_00sec_-10_00C_LIGHT_0541_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20_00sec_-15_00C_LIGHT_0543_fits__*pix.png resample_wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20_00sec_-10_00C_LIGHT_0540_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: 2461093.96521309 22.02.2026 11:09:44.411 /data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits
First image: 2461093.96521309 22.02.2026 11:09:44.411 /data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits
Last image: 2461125.79126124 26.03.2026 06:59:14.971 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.55
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 7574
Objects passed selection criteria: 7559
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 6708
Average stars matched: 6582.25 (98.1254 %)
Memory usage VmPeak: 114164 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 26 02:03:03 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: 2461093.96521309 22.02.2026 11:09:44.411 /data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits
First image: 2461093.96521309 22.02.2026 11:09:44.411 /data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits
Last image: 2461125.79126124 26.03.2026 06:59:14.971 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 41
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.24
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: 19 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): 48204
Objects passed selection criteria: 48101
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 43284.8
Average stars matched: 42085.5 (97.2294 %)
Memory usage VmPeak: 151764 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 26 02:03:56 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/Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits
SExtractor catalog cache: saved Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits.cat to cache
SExtractor catalog cache: saved Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.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/Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461125.79070543
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits exists and is non-empty
Saving wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits to local_wcs_cache/
'wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits' -> 'local_wcs_cache/wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits'
wcs_Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits exists and is non-empty
Saving wcs_Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits to local_wcs_cache/
'wcs_Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits' -> 'local_wcs_cache/wcs_Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits'
wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits exists and is non-empty
Saving wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits to local_wcs_cache/
'wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits' -> 'local_wcs_cache/wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits'
wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits exists and is non-empty
Saving wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits to local_wcs_cache/
'wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits' -> 'local_wcs_cache/wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.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 16:00:00.715 +14:00:06.79
Second-epoch image center 16:00:09.682 +13:58:49.87
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 16:00:00.715 +14:00:06.79
Second-epoch image center 16:00:09.139 +13:58:13.00
Angular distance between the image centers 0.05 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 16:00:09.682 +13:58:49.87
Second-epoch second image center 16:00:09.139 +13:58:13.00
Angular distance between the image centers 0.01047 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/Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits &> /tmp/tmp.CmZtlvQEbb
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits &> /tmp/tmp.TBDLNWMjOj
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits &> /tmp/tmp.gauoCGGf0a
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits &> /tmp/tmp.GeoDb3mjV7
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits
Calibrating the magnitude scale
Found non-empty wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.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_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits and wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.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_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits and wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits.cat
Found non-empty wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits and wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits.cat
The reference image (wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits) and catalog (wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits.cat) found
'wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.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 4713 out of 9866 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.947648
a=0.000000 b=1.000000 c=22.947648
From vast_summary.log: estimated ref. image limiting mag.: -7.55
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.40
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.40
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits
2.2 pix Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits
2.5 pix fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits
2.5 pix fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits
Limiting magnitude estimates:
15.4 mag. Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits
15.4 mag. Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits
14.8 mag. fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits
14.8 mag. fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 11.9 (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.CmZtlvQEbb (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/Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits' -> 'wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits
WCS_IMAGE_NAME=wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits
WCS-calibrated image found: wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits
Checking if the catalog wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits.cat corresponding to the image wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits alredy exist and is non-empty...
Catalog wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits.cat corresponding to the image wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits
WCS catalog name: wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=644, passed=9866
Got 9866 stars (including 9205 good ones) from the SExtractor catalog wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits.cat
util/solve_plate_with_UCAC5 got 9866 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 969 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: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
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 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.30"
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits -region wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.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.TBDLNWMjOj (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/Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits' -> 'wcs_Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits
WCS_IMAGE_NAME=wcs_Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits
WCS-calibrated image found: wcs_Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits
Checking if the catalog wcs_Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits.cat corresponding to the image wcs_Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits alredy exist and is non-empty...
Catalog wcs_Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits.cat corresponding to the image wcs_Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits
WCS catalog name: wcs_Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=650, passed=9873
Got 9873 stars (including 9209 good ones) from the SExtractor catalog wcs_Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits.cat
util/solve_plate_with_UCAC5 got 9873 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 971 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: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
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 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.29"
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits -region wcs_Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.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.gauoCGGf0a (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits
WCS_IMAGE_NAME=wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits
WCS-calibrated image found: wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits
Checking if the catalog wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits.cat corresponding to the image wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits alredy exist and is non-empty...
Catalog wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits.cat corresponding to the image wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits
WCS catalog name: wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=404, passed=6836
Got 6836 stars (including 6426 good ones) from the SExtractor catalog wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits.cat
util/solve_plate_with_UCAC5 got 6836 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 969 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: 0.47"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits -region wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.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.GeoDb3mjV7 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits
WCS_IMAGE_NAME=wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits
WCS-calibrated image found: wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits
Checking if the catalog wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits.cat corresponding to the image wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits alredy exist and is non-empty...
Catalog wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits.cat corresponding to the image wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits
WCS catalog name: wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=404, passed=6852
Got 6852 stars (including 6445 good ones) from the SExtractor catalog wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits.cat
util/solve_plate_with_UCAC5 got 6852 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.47"
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 969 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: 0.46"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits -region wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.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_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits'
Saving fully-calibrated image wcs_Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/wcs_Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits'
Saving fully-calibrated image wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits'
Saving fully-calibrated image wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits'
Preparing the HTML report for the field Ser-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20477.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20420_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541
The candidate 20420_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541 did not pass the final checks
**** FOUND 15:59:47.87 +17:22:48.8 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20477_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541
The candidate 20477_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541 did not pass the final checks
**** FOUND 16:16:05.85 +14:25:49.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.11, MAG_FAINT_SEARCH_LIMIT=13.09)GAIADR2_OUTPUT=# 0.620 4464367918620158208 244.02422432862 +14.43038063661 12.0503 11.7169 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.620#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06003_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541
The candidate 06003_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541 did not pass the final checks
**** FOUND 15:50:41.85 +15:07:59.2 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Ser-02-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/Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits
SExtractor catalog cache: saved Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits.cat to cache
SExtractor catalog cache: saved Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits
Creating symlink local_wcs_cache/wcs_Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits
Creating symlink local_wcs_cache/wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits
Creating symlink local_wcs_cache/wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.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_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits exists and is non-empty
wcs_Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits exists and is non-empty
wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits exists and is non-empty
wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.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 16:00:00.715 +14:00:06.79
Second-epoch image center 16:00:09.682 +13:58:49.87
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 16:00:00.715 +14:00:06.79
Second-epoch image center 16:00:09.139 +13:58:13.00
Angular distance between the image centers 0.05 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 16:00:09.682 +13:58:49.87
Second-epoch second image center 16:00:09.139 +13:58:13.00
Angular distance between the image centers 0.01047 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/Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits &> /tmp/tmp.HvRYahJhs0
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits &> /tmp/tmp.PNoUZc9URZ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits &> /tmp/tmp.VN1mrj65Xc
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits &> /tmp/tmp.v39NvbPOFg
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits
Calibrating the magnitude scale
Found non-empty wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.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_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits and wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.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_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits and wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits.cat
Found non-empty wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits and wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits.cat
The reference image (wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits) and catalog (wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits.cat) found
'wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.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 4755 out of 59899 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.825972
a=0.000000 b=1.000000 c=22.825972
From vast_summary.log: estimated ref. image limiting mag.: -7.24
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.59
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.59
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 31 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits
2.0 pix Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits
2.2 pix fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits
2.2 pix fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits
Limiting magnitude estimates:
15.6 mag. Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits
15.6 mag. Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits
15.0 mag. fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits
15.0 mag. fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 14.4 (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.HvRYahJhs0 (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/Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits' -> 'wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits
WCS_IMAGE_NAME=wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits
WCS-calibrated image found: wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits
Checking if the catalog wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits.cat corresponding to the image wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits alredy exist and is non-empty...
Catalog wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits.cat corresponding to the image wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits
WCS catalog name: wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits.cat
SExtractor catalog parsing summary: zero_flux=5, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=2828, passed=59880
Got 59880 stars (including 56963 good ones) from the SExtractor catalog wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits.cat
util/solve_plate_with_UCAC5 got 59880 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 967 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: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
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 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits -region wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.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.PNoUZc9URZ (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/Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits' -> 'wcs_Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits
WCS_IMAGE_NAME=wcs_Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits
WCS-calibrated image found: wcs_Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits
Checking if the catalog wcs_Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits.cat corresponding to the image wcs_Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits alredy exist and is non-empty...
Catalog wcs_Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits.cat corresponding to the image wcs_Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits
WCS catalog name: wcs_Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=2795, passed=60056
Got 60056 stars (including 57159 good ones) from the SExtractor catalog wcs_Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits.cat
util/solve_plate_with_UCAC5 got 60056 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (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 0.010462 (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 969 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: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
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 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits -region wcs_Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.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.VN1mrj65Xc (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits
WCS_IMAGE_NAME=wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits
WCS-calibrated image found: wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits
Checking if the catalog wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits.cat corresponding to the image wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits alredy exist and is non-empty...
Catalog wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits.cat corresponding to the image wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits
WCS catalog name: wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=1736, passed=40949
Got 40949 stars (including 39162 good ones) from the SExtractor catalog wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits.cat
util/solve_plate_with_UCAC5 got 40949 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.46"
Estimated accuracy of the plate solution: 0.45"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits -region wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.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.v39NvbPOFg (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits
WCS_IMAGE_NAME=wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits
WCS-calibrated image found: wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits
Checking if the catalog wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits.cat corresponding to the image wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits alredy exist and is non-empty...
Catalog wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits.cat corresponding to the image wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits
WCS catalog name: wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=1725, passed=40880
Got 40880 stars (including 39110 good ones) from the SExtractor catalog wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits.cat
util/solve_plate_with_UCAC5 got 40880 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 967 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: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.44"
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 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.44"
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits -region wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.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_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/wcs_Ser-02-Q2b1x1_2026-02-22_05-09-44_20.00sec_-15.00C_LIGHT_0543.fits
Saving fully-calibrated image wcs_Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/wcs_Ser-02-Q2b1x1_2026-02-22_05-10-41_20.00sec_-14.90C_LIGHT_0544.fits
Saving fully-calibrated image wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-58-26_20.00sec_-10.00C_LIGHT_0540.fits
Saving fully-calibrated image wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ser-02-Q2b1x1_020047_TTUQ2b1x1_29868_hhFLhJct/wcs_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541.fits
Preparing the HTML report for the field Ser-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out74000.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out74010.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out74011.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out74014.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out74017.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out74080.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out74121.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out74223.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out74263.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out74279.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out74284.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out74306.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out74313.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out74401.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out74406.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out74412.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out74427.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out74432.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out74446.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out74478.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out74487.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out33652.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out74152.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 74000_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541
The candidate 74000_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541 did not pass the final checks
**** FOUND 16:18:15.76 +11:56:33.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.69, MAG_FAINT_SEARCH_LIMIT=15.67)GAIADR2_OUTPUT=# 0.828 4457060259402445696 244.56547080375 +11.94284935082 14.3522 13.6852 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.828#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 74010_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541
The candidate 74010_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541 did not pass the final checks
**** FOUND 16:09:38.51 +11:57:12.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.03, MAG_FAINT_SEARCH_LIMIT=15.01)GAIADR2_OUTPUT=# 0.556 4457236318701681408 242.41030120714 +11.95348443889 14.0255 13.4042 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.556#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 74011_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541
The candidate 74011_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541 did not pass the final checks
**** FOUND 16:24:06.15 +16:36:55.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.03, MAG_FAINT_SEARCH_LIMIT=15.01)GAIADR2_OUTPUT=# 0.581 4466570519585821056 246.02549197343 +16.61517874660 13.9677 13.3831 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.581#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 74014_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541
The candidate 74014_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541 did not pass the final checks
**** FOUND 16:15:56.09 +17:54:36.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 1.070 1200517168247097344 243.98347065322 +17.91044275765 13.8221 12.9343 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.070#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 74015_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541
The candidate 74015_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541 did not pass the final checks
**** FOUND 15:47:20.66 +09:47:29.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 74017_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541
The candidate 74017_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541 did not pass the final checks
**** FOUND 15:50:28.58 +11:24:33.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 0.807 1189595375653331072 237.61904187045 +11.40944268548 12.8750 12.1674 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.807#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 74080_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541
The candidate 74080_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541 did not pass the final checks
**** FOUND 15:57:22.79 +14:25:54.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 0.611 1192136828060399872 239.34512826094 +14.43170871408 11.9745 11.2555 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.611#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 74087_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541
The candidate 74087_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541 did not pass the final checks
**** FOUND 16:07:31.69 +09:52:25.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 74099_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541
The candidate 74099_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541 did not pass the final checks
**** FOUND 16:25:16.15 +14:02:04.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 74121_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541
The candidate 74121_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541 did not pass the final checks
**** FOUND 16:24:45.09 +12:11:51.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 1.261 4460115626119898496 246.18822850386 +12.19763699936 12.8181 12.1383 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.261#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 74152_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541
Preparing report for the candidate 74152_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541
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Considering the candidate 74160_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541
The candidate 74160_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541 did not pass the final checks
**** FOUND 16:21:48.05 +13:27:03.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 74197_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541
The candidate 74197_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541 did not pass the final checks
**** FOUND 16:03:18.90 +13:50:14.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 74204_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541
The candidate 74204_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541 did not pass the final checks
**** FOUND 16:16:50.36 +17:23:32.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 74223_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541
The candidate 74223_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541 did not pass the final checks
**** FOUND 15:55:24.97 +14:18:21.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)GAIADR2_OUTPUT=# 1.015 1192506710644093952 238.85388175888 +14.30618001996 13.6776 13.1244 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.015#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 74235_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541
The candidate 74235_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541 did not pass the final checks
**** FOUND 16:07:45.68 +16:14:29.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 74263_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541
The candidate 74263_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541 did not pass the final checks
**** FOUND 15:43:21.43 +11:44:17.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)GAIADR2_OUTPUT=# 3.194 1190228969225623040 235.83901250484 +11.73901073168 14.0884 13.5180 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.194#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 74279_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541
The candidate 74279_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541 did not pass the final checks
**** FOUND 16:24:45.56 +17:56:09.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 0.642 4466987749888632064 246.18985220739 +17.93612194922 14.0538 13.3604 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.642#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 74284_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541
The candidate 74284_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541 did not pass the final checks
**** FOUND 16:00:31.05 +14:37:47.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 0.807 1192111745451465856 240.12957358372 +14.62986539391 13.9789 13.4293 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.807#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 74306_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541
The candidate 74306_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541 did not pass the final checks
**** FOUND 16:04:26.70 +13:23:58.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.25, MAG_FAINT_SEARCH_LIMIT=15.23)GAIADR2_OUTPUT=# 1.282 4458392970574714112 241.11124920557 +13.39928289103 14.4119 13.8396 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.282#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 74313_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541
The candidate 74313_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541 did not pass the final checks
**** FOUND 16:18:58.04 +12:53:42.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.27, MAG_FAINT_SEARCH_LIMIT=15.25)GAIADR2_OUTPUT=# 3.318 4463180450360056832 244.74129122885 +12.89449474432 14.5186 14.0055 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.318#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 74401_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541
The candidate 74401_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541 did not pass the final checks
**** FOUND 16:15:13.72 +14:35:15.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.55, MAG_FAINT_SEARCH_LIMIT=15.53)GAIADR2_OUTPUT=# 0.240 4464421386670947456 243.80709790419 +14.58775317168 15.1745 14.7389 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.240#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 74406_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541
The candidate 74406_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541 did not pass the final checks
**** FOUND 16:16:25.06 +12:39:08.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.71, MAG_FAINT_SEARCH_LIMIT=15.69)GAIADR2_OUTPUT=# 0.215 4463160624790857216 244.10438856590 +12.65230807385 14.6977 14.1890 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.215#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 74412_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541
The candidate 74412_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541 did not pass the final checks
**** FOUND 16:23:47.07 +16:26:29.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.83, MAG_FAINT_SEARCH_LIMIT=15.81)GAIADR2_OUTPUT=# 1.195 4466532483355230720 245.94633463073 +16.44181972972 14.6622 13.8985 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.195#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 74427_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541
The candidate 74427_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541 did not pass the final checks
**** FOUND 16:15:17.81 +15:17:02.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.77, MAG_FAINT_SEARCH_LIMIT=15.75)GAIADR2_OUTPUT=# 0.019 4465055358202770048 243.82421366847 +15.28405592163 14.7016 14.0970 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.019#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 74432_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541
The candidate 74432_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541 did not pass the final checks
**** FOUND 16:01:26.77 +13:04:27.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.92, MAG_FAINT_SEARCH_LIMIT=15.90)GAIADR2_OUTPUT=# 0.688 4457996768430807808 240.36167988351 +13.07419784796 14.9254 14.4248 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.688#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 74446_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541
The candidate 74446_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541 did not pass the final checks
**** FOUND 16:18:27.35 +17:08:48.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.96, MAG_FAINT_SEARCH_LIMIT=15.94)GAIADR2_OUTPUT=# 0.837 1200215554166635392 244.61390864401 +17.14714435423 15.1574 14.4859 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.837#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 74478_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541
The candidate 74478_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541 did not pass the final checks
**** FOUND 16:13:10.37 +15:39:38.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.75, MAG_FAINT_SEARCH_LIMIT=15.73)GAIADR2_OUTPUT=# 2.058 4464755569486077696 243.29268310289 +15.66045557224 14.9139 14.5874 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.058#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 74487_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541
The candidate 74487_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541 did not pass the final checks
**** FOUND 16:01:09.58 +15:15:10.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.93, MAG_FAINT_SEARCH_LIMIT=15.91)GAIADR2_OUTPUT=# 1.158 1192310413458276992 240.28991389961 +15.25256729989 15.0604 14.8021 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.158#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 33652_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541
Preparing report for the candidate 33652_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541
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Considering the candidate 37496_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541
The candidate 37496_fd_Ser-02-Q2b1x1_2026-03-26_01-59-14_20.00sec_-10.00C_LIGHT_0541 did not pass the final checks