This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH
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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461129.6422,13.14,0.05,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
target 20260330.1422 13.14CV 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/Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:16:06.01 -08:49:50.6 ;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_Mon-04-Q2b1x1_2026-01-20_22-43-41_20_00sec_-14_90C_LIGHT_0201_fits__*pix.png resample_wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20_00sec_-10_00C_LIGHT_0105_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20_00sec_-14_90C_LIGHT_0201_fits__*pix.png resample_wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20_00sec_-10_00C_LIGHT_0104_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20_00sec_-14_90C_LIGHT_0201_fits__*pix.png resample_wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20_00sec_-10_00C_LIGHT_0105_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20_00sec_-14_90C_LIGHT_0201_fits__*pix.png resample_wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20_00sec_-10_00C_LIGHT_0104_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 30.1422* 05 39 42.91 -08 09 09.5 10.3 U Ori 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
V1187 Ori,2461129.6422,10.26,0.05,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
V1187 Ori 20260330.1422 10.26CV 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/Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:39:42.91 -08:09:09.5 ;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_Mon-04-Q2b1x1_2026-01-20_22-43-41_20_00sec_-14_90C_LIGHT_0201_fits__*pix.png resample_wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20_00sec_-10_00C_LIGHT_0105_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20_00sec_-14_90C_LIGHT_0201_fits__*pix.png resample_wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20_00sec_-10_00C_LIGHT_0104_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20_00sec_-14_90C_LIGHT_0201_fits__*pix.png resample_wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20_00sec_-10_00C_LIGHT_0105_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20_00sec_-14_90C_LIGHT_0201_fits__*pix.png resample_wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20_00sec_-10_00C_LIGHT_0104_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: 2461061.69712250 21.01.2026 04:43:41.384 /data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits
First image: 2461061.69712250 21.01.2026 04:43:41.384 /data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits
Last image: 2461129.64250322 30.03.2026 03:25:02.278 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.85
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: 3 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): 11720
Objects passed selection criteria: 11666
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 8064.75
Average stars matched: 7606.75 (94.321 %)
Memory usage VmPeak: 117368 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Mar 29 22:39:19 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: 2461061.69712250 21.01.2026 04:43:41.384 /data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits
First image: 2461061.69712250 21.01.2026 04:43:41.384 /data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits
Last image: 2461129.64250322 30.03.2026 03:25:02.278 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 39
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.53
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: 14 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): 74052
Objects passed selection criteria: 73897
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 53942.8
Average stars matched: 50295.5 (93.2387 %)
Memory usage VmPeak: 171572 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Mar 29 22:40:23 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/Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits
SExtractor catalog cache: saved Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits.cat to cache
SExtractor catalog cache: saved Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.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/Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.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: 2461129.64189334
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_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits exists and is non-empty
Saving wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits to local_wcs_cache/
'wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits' -> 'local_wcs_cache/wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits'
wcs_Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits exists and is non-empty
Saving wcs_Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits to local_wcs_cache/
'wcs_Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits' -> 'local_wcs_cache/wcs_Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits'
wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits exists and is non-empty
Saving wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits to local_wcs_cache/
'wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits' -> 'local_wcs_cache/wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits'
wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits exists and is non-empty
Saving wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits to local_wcs_cache/
'wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits' -> 'local_wcs_cache/wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.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 05:59:59.886 -09:59:53.51
Second-epoch image center 06:00:17.374 -09:58:21.65
Angular distance between the image centers 0.08 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 05:59:59.886 -09:59:53.51
Second-epoch image center 06:00:19.876 -09:58:41.49
Angular distance between the image centers 0.08 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 06:00:17.374 -09:58:21.65
Second-epoch second image center 06:00:19.876 -09:58:41.49
Angular distance between the image centers 0.01165 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/Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits &> /tmp/tmp.k8hd3Qizxu
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits &> /tmp/tmp.XAdhKBBcWJ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits &> /tmp/tmp.a1ofxn90oZ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits &> /tmp/tmp.c8QmukjVqG
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits
Calibrating the magnitude scale
Found non-empty wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.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_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits and wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.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_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits and wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits.cat
Found non-empty wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits and wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits.cat
The reference image (wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits) and catalog (wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits.cat) found
'wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.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 8758 out of 14559 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.894699
a=0.000000 b=1.000000 c=22.894699
From vast_summary.log: estimated ref. image limiting mag.: -7.85
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.04
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.04
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits
2.2 pix Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits
2.3 pix fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits
2.3 pix fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits
Limiting magnitude estimates:
15.0 mag. Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits
15.0 mag. Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits
13.8 mag. fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits
13.8 mag. fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 10.9 (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.k8hd3Qizxu (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/Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits' -> 'wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits
WCS_IMAGE_NAME=wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits
WCS-calibrated image found: wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits
Checking if the catalog wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits.cat corresponding to the image wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits alredy exist and is non-empty...
Catalog wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits.cat corresponding to the image wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits
WCS catalog name: wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1273, passed=14559
Got 14559 stars (including 13270 good ones) from the SExtractor catalog wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits.cat
util/solve_plate_with_UCAC5 got 14559 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.32"
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 957 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits -region wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.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.XAdhKBBcWJ (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/Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits' -> 'wcs_Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits
WCS_IMAGE_NAME=wcs_Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits
WCS-calibrated image found: wcs_Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits
Checking if the catalog wcs_Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits.cat corresponding to the image wcs_Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits alredy exist and is non-empty...
Catalog wcs_Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits.cat corresponding to the image wcs_Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits
WCS catalog name: wcs_Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1304, passed=14472
Got 14472 stars (including 13151 good ones) from the SExtractor catalog wcs_Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits.cat
util/solve_plate_with_UCAC5 got 14472 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.31"
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 959 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits -region wcs_Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.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.a1ofxn90oZ (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits
WCS_IMAGE_NAME=wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits
WCS-calibrated image found: wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits
Checking if the catalog wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits.cat corresponding to the image wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits.cat corresponding to the image wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits
WCS catalog name: wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=488, passed=5556
Got 5556 stars (including 5055 good ones) from the SExtractor catalog wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits.cat
util/solve_plate_with_UCAC5 got 5556 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.56"
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 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.57"
Estimated accuracy of the plate solution: 0.61"
Excluding outliers - 943 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits -region wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.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.c8QmukjVqG (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits
WCS_IMAGE_NAME=wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits
WCS-calibrated image found: wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits
Checking if the catalog wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits.cat corresponding to the image wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits.cat corresponding to the image wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits
WCS catalog name: wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=482, passed=5462
Got 5462 stars (including 4978 good ones) from the SExtractor catalog wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits.cat
util/solve_plate_with_UCAC5 got 5462 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.53"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.54"
Estimated accuracy of the plate solution: 0.59"
Excluding outliers - 946 stars left (next iteration limit 1040)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits -region wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.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_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits'
Saving fully-calibrated image wcs_Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/wcs_Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits'
Saving fully-calibrated image wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits'
Saving fully-calibrated image wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits'
Preparing the HTML report for the field Mon-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Mon-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits
SExtractor catalog cache: saved Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits.cat to cache
SExtractor catalog cache: saved Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits /data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits
Creating symlink local_wcs_cache/wcs_Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits
Creating symlink local_wcs_cache/wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.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_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits exists and is non-empty
wcs_Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits exists and is non-empty
wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits exists and is non-empty
wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.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 05:59:59.886 -09:59:53.51
Second-epoch image center 06:00:17.374 -09:58:21.65
Angular distance between the image centers 0.08 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 05:59:59.886 -09:59:53.51
Second-epoch image center 06:00:19.876 -09:58:41.49
Angular distance between the image centers 0.08 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 06:00:17.374 -09:58:21.65
Second-epoch second image center 06:00:19.876 -09:58:41.49
Angular distance between the image centers 0.01165 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/Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits &> /tmp/tmp.WnQbPWELJs
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits &> /tmp/tmp.yHAdVrnCOL
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits &> /tmp/tmp.FXCSpXa66u
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits &> /tmp/tmp.SCtSfML6wh
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits
Calibrating the magnitude scale
Found non-empty wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.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_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits and wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.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_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits and wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits.cat
Found non-empty wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits and wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits.cat
The reference image (wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits) and catalog (wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits.cat) found
'wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.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 9122 out of 89203 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.750833
a=0.000000 b=1.000000 c=22.750833
From vast_summary.log: estimated ref. image limiting mag.: -7.53
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.22
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.22
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 26 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits
2.1 pix Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits
2.2 pix fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits
2.2 pix fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits
Limiting magnitude estimates:
15.2 mag. Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits
15.2 mag. Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits
13.9 mag. fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits
13.9 mag. fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits
All-image limiting magnitude estimate: 13.9 (SNR ) 13.4 (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.WnQbPWELJs (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/Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits' -> 'wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits
WCS_IMAGE_NAME=wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits
WCS-calibrated image found: wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits
Checking if the catalog wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits.cat corresponding to the image wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits alredy exist and is non-empty...
Catalog wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits.cat corresponding to the image wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits
WCS catalog name: wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=6785, passed=89197
Got 89197 stars (including 82252 good ones) from the SExtractor catalog wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits.cat
util/solve_plate_with_UCAC5 got 89197 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.32"
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 957 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits -region wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.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.yHAdVrnCOL (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/Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits' -> 'wcs_Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits
WCS_IMAGE_NAME=wcs_Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits
WCS-calibrated image found: wcs_Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits
Checking if the catalog wcs_Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits.cat corresponding to the image wcs_Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits alredy exist and is non-empty...
Catalog wcs_Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits.cat corresponding to the image wcs_Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits
WCS catalog name: wcs_Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=6764, passed=88880
Got 88880 stars (including 81947 good ones) from the SExtractor catalog wcs_Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits.cat
util/solve_plate_with_UCAC5 got 88880 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.32"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits -region wcs_Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.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.FXCSpXa66u (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits
WCS_IMAGE_NAME=wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits
WCS-calibrated image found: wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits
Checking if the catalog wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits.cat corresponding to the image wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits.cat corresponding to the image wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits
WCS catalog name: wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=1841, passed=38108
Got 38108 stars (including 36188 good ones) from the SExtractor catalog wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits.cat
util/solve_plate_with_UCAC5 got 38108 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.51"
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 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.51"
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 945 stars left (next iteration limit 1039)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits -region wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.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.SCtSfML6wh (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits
WCS_IMAGE_NAME=wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits
WCS-calibrated image found: wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits
Checking if the catalog wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits.cat corresponding to the image wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits alredy exist and is non-empty...
Catalog wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits.cat corresponding to the image wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits
WCS catalog name: wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=1753, passed=37628
Got 37628 stars (including 35807 good ones) from the SExtractor catalog wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits.cat
util/solve_plate_with_UCAC5 got 37628 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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 947 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: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.51"
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 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.51"
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 945 stars left (next iteration limit 1039)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits -region wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.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_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/wcs_Mon-04-Q2b1x1_2026-01-20_22-43-41_20.00sec_-14.90C_LIGHT_0201.fits
Saving fully-calibrated image wcs_Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/wcs_Mon-04-Q2b1x1_2026-01-20_22-44-28_20.00sec_-15.00C_LIGHT_0202.fits
Saving fully-calibrated image wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-24-09_20.00sec_-10.00C_LIGHT_0104.fits
Saving fully-calibrated image wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Mon-04-Q2b1x1_223705_TTUQ2b1x1_24102_AHz545xH/wcs_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105.fits
Preparing the HTML report for the field Mon-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out104949.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out104959.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out104968.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out109154.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out109203.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out109245.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out109390.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out110512.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out110567.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out85457.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 14s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 104949_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105
The candidate 104949_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105 did not pass the final checks
**** FOUND 06:02:42.79 -09:18:10.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)GAIADR2_OUTPUT=# 0.396 3005434362156520320 090.67830902048 -09.30299745542 13.6310 13.0003 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.396#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 104955_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105
The candidate 104955_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105 did not pass the final checks
**** FOUND 05:56:30.12 -07:56:07.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 104959_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105
The candidate 104959_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105 did not pass the final checks
**** FOUND 06:04:42.63 -13:07:33.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 1.099 2997350237274368384 091.17732552356 -13.12617308037 13.0929 12.3114 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.099#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 104966_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105
The candidate 104966_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105 did not pass the final checks
**** FOUND 06:11:25.71 -11:30:55.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 104968_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105
The candidate 104968_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105 did not pass the final checks
**** FOUND 06:15:57.11 -07:38:30.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 1.055 3007378225698476800 093.98777305823 -07.64192281112 12.1346 11.6496 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.055#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107302_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105
The candidate 107302_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105 did not pass the final checks
**** FOUND 06:22:41.06 -08:57:36.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 107543_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105
The candidate 107543_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105 did not pass the final checks
**** FOUND 06:01:49.19 -10:37:34.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 107860_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105
The candidate 107860_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105 did not pass the final checks
**** FOUND 06:10:43.86 -10:31:13.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 108145_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105
The candidate 108145_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105 did not pass the final checks
**** FOUND 05:47:07.20 -12:47:45.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 108324_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105
The candidate 108324_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105 did not pass the final checks
**** FOUND 06:20:02.45 -07:51:11.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 108505_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105
The candidate 108505_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105 did not pass the final checks
**** FOUND 06:21:44.42 -08:48:38.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 108645_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105
The candidate 108645_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105 did not pass the final checks
**** FOUND 05:56:30.70 -14:10:54.1 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 109154_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105
The candidate 109154_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105 did not pass the final checks
**** FOUND 06:15:33.03 -07:08:20.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 1.088 3007621943620593536 093.88784517813 -07.13892989843 12.7542 11.9658 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.088#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 109203_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105
The candidate 109203_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105 did not pass the final checks
**** FOUND 06:17:42.71 -07:53:18.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 2.115 3007331603831567744 094.42854822624 -07.88832840883 12.6778 11.7050 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.115#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 109245_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105
The candidate 109245_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105 did not pass the final checks
**** FOUND 06:13:14.49 -09:53:23.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 1.651 3004768156893689344 093.30997485320 -09.89009544115 13.0499 12.5943 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.651#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 109390_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105
The candidate 109390_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105 did not pass the final checks
**** FOUND 05:59:55.79 -08:07:15.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 2.291 3017842522675333376 089.98218450683 -08.12149236891 12.8692 12.3846 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.291#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 109753_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105
The candidate 109753_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105 did not pass the final checks
**** FOUND 06:18:46.54 -09:25:01.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 110512_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105
The candidate 110512_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105 did not pass the final checks
**** FOUND 06:11:42.44 -10:55:53.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 0.805 3004036882878604032 092.92665671764 -10.93146991181 13.1097 12.2284 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.805#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 110567_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105
Preparing report for the candidate 110567_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105
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Considering the candidate 111203_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105
The candidate 111203_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105 did not pass the final checks
**** FOUND 06:05:32.86 -10:15:36.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 111357_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105
The candidate 111357_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105 did not pass the final checks
**** FOUND 06:01:04.44 -12:12:19.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 111458_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105
The candidate 111458_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105 did not pass the final checks
**** FOUND 06:19:37.68 -07:42:40.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 111543_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105
The candidate 111543_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105 did not pass the final checks
**** FOUND 06:15:18.53 -06:25:56.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 111567_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105
The candidate 111567_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105 did not pass the final checks
**** FOUND 06:20:59.40 -08:06:32.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 85457_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105
Preparing report for the candidate 85457_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105
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Considering the candidate 44947_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105
The candidate 44947_fd_Mon-04-Q2b1x1_2026-03-29_22-25-02_20.00sec_-10.00C_LIGHT_0105 did not pass the final checks