This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT
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 04 17.2674* 12 37 51.44 +15 13 24.0 12.3 U Com 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461147.7674,12.27,0.05,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 20260417.2674 12.27CV 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
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 04 17.2674* 12 21 38.82 +15 44 43.2 14.5 U Com 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J185.4116+15.7450,2461147.7674,14.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J185.4116+15.7450 20260417.2674 14.54CV 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
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 04 17.2674* 12 16 37.77 +09 41 13.1 14.5 U Vir 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461147.7674,14.49,0.05,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 20260417.2674 14.49CV 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461098.86697102 27.02.2026 08:48:16.296 /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits
First image: 2461098.86697102 27.02.2026 08:48:16.296 /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits
Last image: 2461147.76773094 17.04.2026 06:25:21.953 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.98
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: 2 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): 4080
Objects passed selection criteria: 4077
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 3855
Average stars matched: 3659.75 (94.9351 %)
Memory usage VmPeak: 110496 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Apr 17 01:30:43 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: 2461098.86697102 27.02.2026 08:48:16.296 /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits
First image: 2461098.86697102 27.02.2026 08:48:16.296 /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits
Last image: 2461147.76773094 17.04.2026 06:25:21.953 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 74
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.72
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: 10 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): 21339
Objects passed selection criteria: 21266
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 20057
Average stars matched: 18502.5 (92.2496 %)
Memory usage VmPeak: 125352 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Apr 17 01:31:21 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/Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits
SExtractor catalog cache: saved Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits.cat to cache
SExtractor catalog cache: saved Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.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/Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.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: 2461147.76705605
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits exists and is non-empty
Saving wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits to local_wcs_cache/
'wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits' -> 'local_wcs_cache/wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits'
wcs_Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits exists and is non-empty
Saving wcs_Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits to local_wcs_cache/
'wcs_Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits' -> 'local_wcs_cache/wcs_Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits'
wcs_fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits exists and is non-empty
Saving wcs_fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits to local_wcs_cache/
'wcs_fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits' -> 'local_wcs_cache/wcs_fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits'
wcs_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits exists and is non-empty
Saving wcs_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits to local_wcs_cache/
'wcs_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits' -> 'local_wcs_cache/wcs_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits (1st reference image)
verification OK: wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits
Image size: 937.2'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 12:27:03.208 +14:00:25.81 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits (1st new image)
verification OK: wcs_fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 12:26:43.814 +14:00:27.63 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 12:27:03.208 +14:00:25.81
Second-epoch image center 12:26:43.814 +14:00:27.63
Angular distance between the image centers 0.0784 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits (2nd new image)
verification OK: wcs_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 12:26:41.763 +13:59:45.82 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 12:27:03.208 +14:00:25.81
Second-epoch image center 12:26:41.763 +13:59:45.82
Angular distance between the image centers 0.0874 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 12:26:43.814 +14:00:27.63
Second-epoch second image center 12:26:41.763 +13:59:45.82
Angular distance between the image centers 0.01427 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/Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits &> /tmp/tmp.a2uxi8JIbN
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits &> /tmp/tmp.i1KSJFD8nD
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits &> /tmp/tmp.X6wsqOs3qw
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits &> /tmp/tmp.IhUNoT4p7y
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits
Calibrating the magnitude scale
Found non-empty wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.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_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits and wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.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_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits and wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits.cat
Found non-empty wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits and wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits.cat
The reference image (wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits) and catalog (wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits.cat) found
'wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits.cat' -> 'wcsmag.cat'
Read 4609 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 178.5626 to 195.0511 deg, Dec +8.6441 to +19.2662 deg
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
Tycho-2 catalog search boundaries: RA 178.5626 to 195.0511 deg, Dec 8.6441 to 19.2662 deg
Loaded 3629 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 2887 out of 2967 total matches.
Matched with Tycho-2 2967 out of 4609 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.987766
a=0.000000 b=1.000000 c=22.987766
From vast_summary.log: estimated ref. image limiting mag.: -7.98
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.01
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.01
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.5 pix Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits
2.5 pix Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits
2.5 pix fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits
2.4 pix fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits
Limiting magnitude estimates:
15.0 mag. Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits
15.0 mag. Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits
15.3 mag. fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits
15.3 mag. fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits
All-image limiting magnitude estimate: 15.3 (SNR ) 12.1 (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.a2uxi8JIbN (6) ############
Parsing command line arguments...
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_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits' -> 'wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits
WCS_IMAGE_NAME=wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits
WCS-calibrated image found: wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits
Checking if the catalog wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits.cat corresponding to the image wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits alredy exist and is non-empty...
Catalog wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits.cat corresponding to the image wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits
WCS catalog name: wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=280, passed=4609
Got 4609 stars (including 4324 good ones) from the SExtractor catalog wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits.cat
util/solve_plate_with_UCAC5 got 4609 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (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...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 967 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 4555 with non-zero local correction accuracy
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...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 4554 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 4554 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits -region wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.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.i1KSJFD8nD (6) ############
Parsing command line arguments...
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_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits' -> 'wcs_Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits
WCS_IMAGE_NAME=wcs_Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits
WCS-calibrated image found: wcs_Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits
Checking if the catalog wcs_Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits.cat corresponding to the image wcs_Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits alredy exist and is non-empty...
Catalog wcs_Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits.cat corresponding to the image wcs_Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits
WCS catalog name: wcs_Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=296, passed=4588
Got 4588 stars (including 4288 good ones) from the SExtractor catalog wcs_Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits.cat
util/solve_plate_with_UCAC5 got 4588 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (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...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 968 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 4540 with non-zero local correction accuracy
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...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 4541 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 4541 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits -region wcs_Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.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.X6wsqOs3qw (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_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.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_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits
WCS_IMAGE_NAME=wcs_fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits
WCS-calibrated image found: wcs_fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits
Checking if the catalog wcs_fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits.cat corresponding to the image wcs_fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits alredy exist and is non-empty...
Catalog wcs_fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits.cat corresponding to the image wcs_fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits
WCS catalog name: wcs_fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=329, passed=5402
Got 5402 stars (including 5072 good ones) from the SExtractor catalog wcs_fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits.cat
util/solve_plate_with_UCAC5 got 5402 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (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...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 966 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 5350 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 5349 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 5349 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits -region wcs_fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.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.IhUNoT4p7y (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_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.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_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits
WCS_IMAGE_NAME=wcs_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits
WCS-calibrated image found: wcs_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits
Checking if the catalog wcs_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits.cat corresponding to the image wcs_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits alredy exist and is non-empty...
Catalog wcs_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits.cat corresponding to the image wcs_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits
WCS catalog name: wcs_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=331, passed=5394
Got 5394 stars (including 5058 good ones) from the SExtractor catalog wcs_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits.cat
util/solve_plate_with_UCAC5 got 5394 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (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...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 965 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 5331 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
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...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 5332 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 5332 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits -region wcs_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.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_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits'
Saving fully-calibrated image wcs_Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/wcs_Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits'
Saving fully-calibrated image wcs_fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/wcs_fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits'
Saving fully-calibrated image wcs_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/wcs_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits'
Preparing the HTML report for the field Com-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20198_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206
The candidate 20198_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206 did not pass the final checks
**** FOUND 12:18:49.84 +14:25:00.2 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Com-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits
SExtractor catalog cache: saved Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits.cat to cache
SExtractor catalog cache: saved Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits
Creating symlink local_wcs_cache/wcs_Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits
Creating symlink local_wcs_cache/wcs_fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits
Creating symlink local_wcs_cache/wcs_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.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_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits exists and is non-empty
wcs_Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits exists and is non-empty
wcs_fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits exists and is non-empty
wcs_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits (1st reference image)
verification OK: wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits
Image size: 937.2'x624.2' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 12:27:03.208 +14:00:25.81 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits (1st new image)
verification OK: wcs_fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 12:26:43.814 +14:00:27.63 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 12:27:03.208 +14:00:25.81
Second-epoch image center 12:26:43.814 +14:00:27.63
Angular distance between the image centers 0.0784 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits (2nd new image)
verification OK: wcs_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits
Image size: 937.2'x624.1' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 12:26:41.763 +13:59:45.82 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 12:27:03.208 +14:00:25.81
Second-epoch image center 12:26:41.763 +13:59:45.82
Angular distance between the image centers 0.0874 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 12:26:43.814 +14:00:27.63
Second-epoch second image center 12:26:41.763 +13:59:45.82
Angular distance between the image centers 0.01427 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/Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits &> /tmp/tmp.3G0nAGrtev
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits &> /tmp/tmp.xruDSAcO4U
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits &> /tmp/tmp.7yPZL2bJ5f
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits &> /tmp/tmp.cI4s2geVUV
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits
Calibrating the magnitude scale
Found non-empty wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.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_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits and wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.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_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits and wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits.cat
Found non-empty wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits and wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits.cat
The reference image (wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits) and catalog (wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits.cat) found
'wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits.cat' -> 'wcsmag.cat'
Read 21947 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 178.5627 to 195.0761 deg, Dec +8.6130 to +19.2739 deg
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
Tycho-2 catalog search boundaries: RA 178.5627 to 195.0761 deg, Dec 8.6130 to 19.2739 deg
Loaded 3648 Tycho-2 stars within the image boundaries (VT and BT non-zero).
Relation between the catalog and instrumental magnitudes is written to calib.txt
Stars used for magnitude calibration (good matches): 2878 out of 3041 total matches.
Matched with Tycho-2 3041 out of 21947 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.871056
a=0.000000 b=1.000000 c=22.871056
From vast_summary.log: estimated ref. image limiting mag.: -7.72
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.15
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.15
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 30 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.4 pix Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits
2.4 pix Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits
2.2 pix fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits
2.2 pix fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits
Limiting magnitude estimates:
15.1 mag. Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits
15.2 mag. Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits
15.4 mag. fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits
15.4 mag. fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits
All-image limiting magnitude estimate: 15.4 (SNR ) 14.5 (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.3G0nAGrtev (6) ############
Parsing command line arguments...
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_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits' -> 'wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits
WCS_IMAGE_NAME=wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits
WCS-calibrated image found: wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits
Checking if the catalog wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits.cat corresponding to the image wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits alredy exist and is non-empty...
Catalog wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits.cat corresponding to the image wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits
WCS catalog name: wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=827, passed=21939
Got 21939 stars (including 21087 good ones) from the SExtractor catalog wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits.cat
util/solve_plate_with_UCAC5 got 21939 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (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...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 967 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 21701 with non-zero local correction accuracy
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...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 21701 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 21701 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 979 stars left (next iteration limit 1076)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits -region wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.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.xruDSAcO4U (6) ############
Parsing command line arguments...
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_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits' -> 'wcs_Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits
WCS_IMAGE_NAME=wcs_Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits
WCS-calibrated image found: wcs_Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits
Checking if the catalog wcs_Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits.cat corresponding to the image wcs_Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits alredy exist and is non-empty...
Catalog wcs_Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits.cat corresponding to the image wcs_Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits
WCS catalog name: wcs_Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=906, passed=22390
Got 22390 stars (including 21458 good ones) from the SExtractor catalog wcs_Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits.cat
util/solve_plate_with_UCAC5 got 22390 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (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...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 970 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 22144 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 22145 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 22145 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 979 stars left (next iteration limit 1076)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits -region wcs_Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.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.7yPZL2bJ5f (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_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.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_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits
WCS_IMAGE_NAME=wcs_fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits
WCS-calibrated image found: wcs_fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits
Checking if the catalog wcs_fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits.cat corresponding to the image wcs_fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits alredy exist and is non-empty...
Catalog wcs_fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits.cat corresponding to the image wcs_fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits
WCS catalog name: wcs_fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=1128, passed=26909
Got 26909 stars (including 25748 good ones) from the SExtractor catalog wcs_fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits.cat
util/solve_plate_with_UCAC5 got 26909 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (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...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 970 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 26640 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 26638 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 26637 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 978 stars left (next iteration limit 1075)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits -region wcs_fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.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.cI4s2geVUV (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_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.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_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits
WCS_IMAGE_NAME=wcs_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits
WCS-calibrated image found: wcs_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits
Checking if the catalog wcs_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits.cat corresponding to the image wcs_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits alredy exist and is non-empty...
Catalog wcs_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits.cat corresponding to the image wcs_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits
WCS catalog name: wcs_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=1138, passed=26935
Got 26935 stars (including 25761 good ones) from the SExtractor catalog wcs_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits.cat
util/solve_plate_with_UCAC5 got 26935 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (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...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 971 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 26670 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 978 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 26669 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 978 matched stars entering correct_measured_positions(), 26669 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 978 stars left (next iteration limit 1075)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits -region wcs_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.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_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.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_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/wcs_Com-04-Q2b1x1_2026-02-27_02-48-16_20.00sec_-15.00C_LIGHT_0138.fits
Saving fully-calibrated image wcs_Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.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_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/wcs_Com-04-Q2b1x1_2026-02-27_02-48-57_20.00sec_-15.00C_LIGHT_0139.fits
Saving fully-calibrated image wcs_fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.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_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/wcs_fd_Com-04-Q2b1x1_2026-04-17_01-24-23_20.00sec_-4.90C_LIGHT_0205.fits
Saving fully-calibrated image wcs_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.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_2026-04-17_CI_Com-04-Q2b1x1_012642_TTUQ2b1x1_75024_zVTuZipT/wcs_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206.fits
Preparing the HTML report for the field Com-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out31441.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out31791.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out31715.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out31501.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31680.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out31702.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 14s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31440_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206
The candidate 31440_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206 did not pass the final checks
**** FOUND 12:36:44.78 +17:29:32.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31441_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206
The candidate 31441_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206 did not pass the final checks
**** FOUND 12:28:32.07 +14:32:14.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.51, MAG_FAINT_SEARCH_LIMIT=15.49)GAIADR2_OUTPUT=# 1.932 3933003571306150144 187.13332222727 +14.53699491346 14.5549 13.8788 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.932#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31501_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206
Preparing report for the candidate 31501_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31527_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206
The candidate 31527_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206 did not pass the final checks
**** FOUND 12:37:32.26 +17:49:08.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31532_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206
The candidate 31532_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206 did not pass the final checks
**** FOUND 12:38:53.40 +16:12:55.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31535_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206
The candidate 31535_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206 did not pass the final checks
**** FOUND 12:20:01.44 +10:31:02.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31569_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206
The candidate 31569_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206 did not pass the final checks
**** FOUND 12:16:36.19 +14:18:23.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31671_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206
The candidate 31671_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206 did not pass the final checks
**** FOUND 12:43:07.81 +12:03:00.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31676_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206
The candidate 31676_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206 did not pass the final checks
**** FOUND 12:23:19.90 +15:49:13.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31680_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206
Preparing report for the candidate 31680_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31688_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206
The candidate 31688_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206 did not pass the final checks
**** FOUND 12:37:41.81 +18:13:39.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31692_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206
The candidate 31692_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206 did not pass the final checks
**** FOUND 12:54:42.86 +18:02:45.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31694_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206
The candidate 31694_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206 did not pass the final checks
**** FOUND 12:46:46.29 +09:51:01.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31697_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206
The candidate 31697_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206 did not pass the final checks
**** FOUND 12:11:15.16 +17:53:17.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31702_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206
Preparing report for the candidate 31702_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31706_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206
The candidate 31706_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206 did not pass the final checks
**** FOUND 12:12:11.85 +13:14:49.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31710_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206
The candidate 31710_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206 did not pass the final checks
**** FOUND 12:52:21.35 +18:06:11.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31715_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206
The candidate 31715_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206 did not pass the final checks
**** FOUND 12:40:23.91 +11:05:52.7 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.48, MAG_FAINT_SEARCH_LIMIT=15.46)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31723_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206
The candidate 31723_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206 did not pass the final checks
**** FOUND 12:09:38.88 +17:57:32.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31724_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206
The candidate 31724_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206 did not pass the final checks
**** FOUND 12:14:27.49 +10:39:29.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31733_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206
The candidate 31733_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206 did not pass the final checks
**** FOUND 12:32:03.36 +16:41:17.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31749_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206
The candidate 31749_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206 did not pass the final checks
**** FOUND 12:24:46.42 +10:05:02.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31755_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206
The candidate 31755_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206 did not pass the final checks
**** FOUND 12:46:43.30 +14:43:30.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31759_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206
The candidate 31759_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206 did not pass the final checks
**** FOUND 12:30:56.86 +12:25:26.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31760_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206
The candidate 31760_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206 did not pass the final checks
**** FOUND 12:48:42.11 +12:27:08.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31791_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206
The candidate 31791_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206 did not pass the final checks
**** FOUND 12:52:21.13 +16:31:23.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.71, MAG_FAINT_SEARCH_LIMIT=15.69)GAIADR2_OUTPUT=# 1.435 3934522954641121792 193.08779382003 +16.52298561725 14.6111 14.0309 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.435#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31794_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206
The candidate 31794_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206 did not pass the final checks
**** FOUND 12:42:25.38 +15:22:40.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31798_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206
The candidate 31798_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206 did not pass the final checks
**** FOUND 12:54:42.52 +17:47:34.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31800_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206
The candidate 31800_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206 did not pass the final checks
**** FOUND 12:45:24.62 +17:42:11.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31833_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206
The candidate 31833_fd_Com-04-Q2b1x1_2026-04-17_01-25-21_20.00sec_-5.00C_LIGHT_0206 did not pass the final checks