This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 30.1434* 05 00 58.36 +05 04 43.8 12.8 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
VARIABLE_NAME,2461129.6434,12.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260330.1434 12.77CV 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/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:00:58.36 +05:04:43.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20_00sec_-14_90C_LIGHT_0159_fits__*pix.png resample_wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20_00sec_-10_00C_LIGHT_0107_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20_00sec_-14_90C_LIGHT_0159_fits__*pix.png resample_wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20_00sec_-10_00C_LIGHT_0106_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20_00sec_-14_90C_LIGHT_0159_fits__*pix.png resample_wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20_00sec_-10_00C_LIGHT_0107_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20_00sec_-14_90C_LIGHT_0159_fits__*pix.png resample_wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20_00sec_-10_00C_LIGHT_0106_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 30.1434* 05 15 32.43 +09 24 34.8 9.2 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
EV Ori,2461129.6434,9.20,0.05,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
EV Ori 20260330.1434 9.20CV 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/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:15:32.43 +09:24:34.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20_00sec_-14_90C_LIGHT_0159_fits__*pix.png resample_wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20_00sec_-10_00C_LIGHT_0107_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20_00sec_-14_90C_LIGHT_0159_fits__*pix.png resample_wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20_00sec_-10_00C_LIGHT_0106_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20_00sec_-14_90C_LIGHT_0159_fits__*pix.png resample_wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20_00sec_-10_00C_LIGHT_0107_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20_00sec_-14_90C_LIGHT_0159_fits__*pix.png resample_wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20_00sec_-10_00C_LIGHT_0106_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.68831204 09.01.2026 04:31:00.160 /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
First image: 2461049.68831204 09.01.2026 04:31:00.160 /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
Last image: 2461129.64379133 30.03.2026 03:26:53.571 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.61
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): 13420
Objects passed selection criteria: 13348
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 8929.25
Average stars matched: 8437.75 (94.4956 %)
Memory usage VmPeak: 118932 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 22:35:20 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.68831204 09.01.2026 04:31:00.160 /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
First image: 2461049.68831204 09.01.2026 04:31:00.160 /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
Last image: 2461129.64379133 30.03.2026 03:26:53.571 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 32
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.27
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: 15 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): 89109
Objects passed selection criteria: 88860
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: 61575.2
Average stars matched: 57809.8 (93.8847 %)
Memory usage VmPeak: 1994712 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 22:36:35 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/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits
SExtractor catalog cache: saved Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits.cat to cache
SExtractor catalog cache: saved Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.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/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.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: 2461129.64302682
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits exists and is non-empty
Saving wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits to local_wcs_cache/
'wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits' -> 'local_wcs_cache/wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits'
wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits exists and is non-empty
Saving wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits to local_wcs_cache/
'wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits' -> 'local_wcs_cache/wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits'
wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits exists and is non-empty
Saving wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits to local_wcs_cache/
'wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits' -> 'local_wcs_cache/wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits'
wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits exists and is non-empty
Saving wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits to local_wcs_cache/
'wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits' -> 'local_wcs_cache/wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.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 05:08:30.148 +06:00:49.89
Second-epoch image center 05:08:44.036 +05:59:58.08
Angular distance between the image centers 0.06 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 05:08:30.148 +06:00:49.89
Second-epoch image center 05:08:41.042 +05:59:34.88
Angular distance between the image centers 0.05 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 05:08:44.036 +05:59:58.08
Second-epoch second image center 05:08:41.042 +05:59:34.88
Angular distance between the image centers 0.01398 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/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits &> /tmp/tmp.weZLzzohJo
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits &> /tmp/tmp.zvXlEGovOq
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits &> /tmp/tmp.eXTl4ku5Ke
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits &> /tmp/tmp.9rWPEHJhCC
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits
Calibrating the magnitude scale
Found non-empty wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.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_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits and wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.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_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits and wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits.cat
Found non-empty wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits and wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits.cat
The reference image (wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits) and catalog (wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits.cat) found
'wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.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 8333 out of 16511 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.928470
a=0.000000 b=1.000000 c=22.928470
From vast_summary.log: estimated ref. image limiting mag.: -7.61
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.32
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.32
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:
2.0 pix Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
2.0 pix Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
2.3 pix fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits
2.3 pix fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits
Limiting magnitude estimates:
15.3 mag. Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
15.3 mag. Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
13.7 mag. fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits
13.7 mag. fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits
All-image limiting magnitude estimate: 13.7 (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.weZLzzohJo (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/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.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_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits' -> 'wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
WCS_IMAGE_NAME=wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
WCS-calibrated image found: wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
Checking if the catalog wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits.cat corresponding to the image wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits alredy exist and is non-empty...
Catalog wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits.cat corresponding to the image wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
WCS catalog name: wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1518, passed=16511
Got 16511 stars (including 14968 good ones) from the SExtractor catalog wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits.cat
util/solve_plate_with_UCAC5 got 16511 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 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: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
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: 0.36"
Estimated accuracy of the plate solution: 0.35"
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_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits -region wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.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.zvXlEGovOq (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/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.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_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits' -> 'wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
WCS_IMAGE_NAME=wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
WCS-calibrated image found: wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
Checking if the catalog wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits.cat corresponding to the image wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits alredy exist and is non-empty...
Catalog wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits.cat corresponding to the image wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
WCS catalog name: wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1534, passed=16525
Got 16525 stars (including 14970 good ones) from the SExtractor catalog wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits.cat
util/solve_plate_with_UCAC5 got 16525 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 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: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 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_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits -region wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.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.eXTl4ku5Ke (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_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.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_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits
WCS_IMAGE_NAME=wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits
WCS-calibrated image found: wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits
Checking if the catalog wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits.cat corresponding to the image wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits.cat corresponding to the image wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.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_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits
WCS catalog name: wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=428, passed=5301
Got 5301 stars (including 4867 good ones) from the SExtractor catalog wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits.cat
util/solve_plate_with_UCAC5 got 5301 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 939 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: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.47"
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 935 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits -region wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.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.9rWPEHJhCC (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_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.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_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits
WCS_IMAGE_NAME=wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits
WCS-calibrated image found: wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits
Checking if the catalog wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits.cat corresponding to the image wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits.cat corresponding to the image wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.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_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits
WCS catalog name: wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=425, passed=5176
Got 5176 stars (including 4748 good ones) from the SExtractor catalog wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits.cat
util/solve_plate_with_UCAC5 got 5176 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
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 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.49"
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 937 stars left (next iteration limit 1030)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits -region wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.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_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits'
Saving fully-calibrated image wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits'
Saving fully-calibrated image wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits'
Saving fully-calibrated image wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits'
Preparing the HTML report for the field Ori-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Ori-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits
SExtractor catalog cache: saved Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits.cat to cache
SExtractor catalog cache: saved Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
Creating symlink local_wcs_cache/wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
Creating symlink local_wcs_cache/wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits
Creating symlink local_wcs_cache/wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.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_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits exists and is non-empty
wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits exists and is non-empty
wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits exists and is non-empty
wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.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 05:08:30.148 +06:00:49.89
Second-epoch image center 05:08:44.036 +05:59:58.08
Angular distance between the image centers 0.06 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 05:08:30.148 +06:00:49.89
Second-epoch image center 05:08:41.042 +05:59:34.88
Angular distance between the image centers 0.05 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 05:08:44.036 +05:59:58.08
Second-epoch second image center 05:08:41.042 +05:59:34.88
Angular distance between the image centers 0.01398 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/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits &> /tmp/tmp.JncGKCaRbp
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits &> /tmp/tmp.ZxP603OoGs
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits &> /tmp/tmp.OUwIGKjJSh
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits &> /tmp/tmp.MmaJ03EHhW
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits
Calibrating the magnitude scale
Found non-empty wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.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_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits and wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.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_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits and wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits.cat
Found non-empty wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits and wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits.cat
The reference image (wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits) and catalog (wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits.cat) found
'wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.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 8494 out of 107661 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.790183
a=0.000000 b=1.000000 c=22.790183
From vast_summary.log: estimated ref. image limiting mag.: -7.27
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.52
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.52
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 25 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
1.9 pix Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
2.2 pix fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits
2.2 pix fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits
Limiting magnitude estimates:
15.5 mag. Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
15.5 mag. Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
13.8 mag. fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits
13.8 mag. fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 13.3 (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.JncGKCaRbp (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/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.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_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits' -> 'wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
WCS_IMAGE_NAME=wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
WCS-calibrated image found: wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
Checking if the catalog wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits.cat corresponding to the image wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits alredy exist and is non-empty...
Catalog wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits.cat corresponding to the image wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
WCS catalog name: wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=27, blended=9183, passed=107634
Got 107634 stars (including 98272 good ones) from the SExtractor catalog wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits.cat
util/solve_plate_with_UCAC5 got 107634 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 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.36"
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 949 stars left (next iteration limit 1043)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits -region wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.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.ZxP603OoGs (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/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.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_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits' -> 'wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
WCS_IMAGE_NAME=wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
WCS-calibrated image found: wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
Checking if the catalog wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits.cat corresponding to the image wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits alredy exist and is non-empty...
Catalog wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits.cat corresponding to the image wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
WCS catalog name: wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=33, blended=9161, passed=107847
Got 107847 stars (including 98493 good ones) from the SExtractor catalog wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits.cat
util/solve_plate_with_UCAC5 got 107847 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 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: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 946 stars left (next iteration limit 1041)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits -region wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.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.OUwIGKjJSh (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_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.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_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits
WCS_IMAGE_NAME=wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits
WCS-calibrated image found: wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits
Checking if the catalog wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits.cat corresponding to the image wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits.cat corresponding to the image wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.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_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits
WCS catalog name: wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=1582, passed=35687
Got 35687 stars (including 34049 good ones) from the SExtractor catalog wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits.cat
util/solve_plate_with_UCAC5 got 35687 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.46"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.47"
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 932 stars left (next iteration limit 1024)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits -region wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.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.MmaJ03EHhW (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_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.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_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits
WCS_IMAGE_NAME=wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits
WCS-calibrated image found: wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits
Checking if the catalog wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits.cat corresponding to the image wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits.cat corresponding to the image wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.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_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits
WCS catalog name: wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=1581, passed=34960
Got 34960 stars (including 33341 good ones) from the SExtractor catalog wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits.cat
util/solve_plate_with_UCAC5 got 34960 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 938 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: 0.51"
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 938 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: 0.48"
Excluding outliers - 934 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits -region wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.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_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.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_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/wcs_Ori-03-Q2b1x1_2026-01-08_22-31-00_20.00sec_-14.90C_LIGHT_0159.fits
Saving fully-calibrated image wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.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_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/wcs_Ori-03-Q2b1x1_2026-01-08_22-31-42_20.00sec_-14.90C_LIGHT_0160.fits
Saving fully-calibrated image wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.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_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-25-47_20.00sec_-10.00C_LIGHT_0106.fits
Saving fully-calibrated image wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.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_Ori-03-Q2b1x1_223304_TTUQ2b1x1_16080_9FuslxRr/wcs_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107.fits
Preparing the HTML report for the field Ori-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out128027.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129274.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out129673.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out131296.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out129515.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out89275.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 4s
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 125053_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107
The candidate 125053_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107 did not pass the final checks
**** FOUND 05:25:16.40 +07:52:32.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125054_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107
The candidate 125054_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107 did not pass the final checks
**** FOUND 05:28:09.52 +04:15:00.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125057_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107
The candidate 125057_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107 did not pass the final checks
**** FOUND 05:17:24.28 +03:53:23.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 127167_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107
The candidate 127167_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107 did not pass the final checks
**** FOUND 05:30:24.63 +04:10:59.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 127179_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107
The candidate 127179_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107 did not pass the final checks
**** FOUND 05:13:22.91 +02:53:53.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 127939_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107
The candidate 127939_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107 did not pass the final checks
**** FOUND 05:30:16.20 +04:52:19.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 128026_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107
The candidate 128026_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107 did not pass the final checks
**** FOUND 05:14:45.51 +05:11:19.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 128027_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107
The candidate 128027_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107 did not pass the final checks
**** FOUND 05:28:55.49 +09:25:13.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 2.417 3338043123550496128 082.23144275796 +09.41967526454 12.5140 11.7370 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.417#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 128104_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107
The candidate 128104_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107 did not pass the final checks
**** FOUND 05:20:59.72 +09:43:45.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 128114_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107
The candidate 128114_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107 did not pass the final checks
**** FOUND 05:26:39.73 +06:53:18.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 128304_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107
The candidate 128304_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107 did not pass the final checks
**** FOUND 05:19:06.04 +02:34:26.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 128310_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107
The candidate 128310_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107 did not pass the final checks
**** FOUND 04:54:55.05 +10:11:06.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 129274_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107
The candidate 129274_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107 did not pass the final checks
**** FOUND 05:30:20.51 +09:46:15.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 3.470 3338078715943567232 082.58528572196 +09.76999556705 13.1681 12.2718 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.470#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129398_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107
The candidate 129398_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107 did not pass the final checks
**** FOUND 04:50:15.16 +06:59:03.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 129515_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107
Preparing report for the candidate 129515_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107
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Considering the candidate 129673_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107
The candidate 129673_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107 did not pass the final checks
**** FOUND 05:22:47.03 +02:46:36.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 2.881 3234419645893775104 080.69617773062 +02.77603582380 12.6355 11.8272 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.881#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 129991_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107
The candidate 129991_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107 did not pass the final checks
**** FOUND 05:14:36.90 +05:10:26.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 130470_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107
The candidate 130470_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107 did not pass the final checks
**** FOUND 05:11:45.01 +05:23:35.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 130669_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107
The candidate 130669_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107 did not pass the final checks
**** FOUND 05:15:10.34 +03:28:37.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 131296_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107
The candidate 131296_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107 did not pass the final checks
**** FOUND 05:24:34.18 +02:48:45.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)GAIADR2_OUTPUT=# 2.753 3235911343870841728 081.14213276070 +02.81201191247 13.7542 13.3160 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.753#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 131979_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107
The candidate 131979_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107 did not pass the final checks
**** FOUND 05:01:08.67 +07:51:54.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 37666_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107
The candidate 37666_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107 did not pass the final checks
**** FOUND 05:00:05.09 +04:27:25.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 89275_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107
Preparing report for the candidate 89275_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107
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Considering the candidate 101230_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107
The candidate 101230_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107 did not pass the final checks
**** FOUND 04:59:00.63 +08:07:49.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 119280_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107
The candidate 119280_fd_Ori-03-Q2b1x1_2026-03-29_22-26-53_20.00sec_-10.00C_LIGHT_0107 did not pass the final checks