This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J160051.32-294140.5,2461150.9120,12.21,0.05,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
ASASSN-V J160051.32-294140.5 20260420.4120 12.21CV 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!
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
ASASSN-V J161516.37-272449.1,2461150.9120,12.56,0.05,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
ASASSN-V J161516.37-272449.1 20260420.4120 12.56CV 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!
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
ASASSN-V J155929.24-294221.2,2461150.9120,11.95,0.05,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
ASASSN-V J155929.24-294221.2 20260420.4120 11.95CV 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: 2461098.96517225 27.02.2026 11:09:40.882 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
First image: 2461098.96517225 27.02.2026 11:09:40.882 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
Last image: 2461150.91239221 20.04.2026 09:53:40.687 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.21
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): 5846
Objects passed selection criteria: 5815
Measurements per detected object (mean, median, min, max): 2.2 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.2 2.0 2 4
Average stars detected per image: 3581.75
Average stars matched: 3299 (92.1058 %)
Memory usage VmPeak: 112548 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 Mon Apr 20 04:55:44 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: 2461098.96517225 27.02.2026 11:09:40.882 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
First image: 2461098.96517225 27.02.2026 11:09:40.882 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
Last image: 2461150.91239221 20.04.2026 09:53:40.687 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 12
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.88
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): 59518
Objects passed selection criteria: 59354
Measurements per detected object (mean, median, min, max): 2.2 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.2 2.0 2 4
Average stars detected per image: 37670
Average stars matched: 34522.5 (91.6445 %)
Memory usage VmPeak: 165188 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 Mon Apr 20 04:57:17 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/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits
SExtractor catalog cache: saved Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat to cache
SExtractor catalog cache: saved Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.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/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.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: 2461150.91162861
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
'asassn_transients_list.txt' -> '../asassn_transients_list.txt'
'tns_transients_list.txt' -> '../tns_transients_list.txt'
wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits exists and is non-empty
Saving wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits to local_wcs_cache/
'wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits' -> 'local_wcs_cache/wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits'
wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits exists and is non-empty
Saving wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits to local_wcs_cache/
'wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits' -> 'local_wcs_cache/wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits'
wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits exists and is non-empty
Saving wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits to local_wcs_cache/
'wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits' -> 'local_wcs_cache/wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits'
wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits exists and is non-empty
Saving wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits to local_wcs_cache/
'wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits' -> 'local_wcs_cache/wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits (1st reference image)
verification OK: wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
Image size: 941.6'x627.5' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 16:19:16.444 -25:59:35.75 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits (1st new image)
verification OK: wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits
Image size: 937.0'x624.4' 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: 16:19:01.945 -25:57:34.94 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 16:19:16.444 -25:59:35.75
Second-epoch image center 16:19:01.945 -25:57:34.94
Angular distance between the image centers 0.0638 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits (2nd new image)
verification OK: wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits
Image size: 937.0'x624.4' 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: 16:19:04.260 -25:57:13.34 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 16:19:16.444 -25:59:35.75
Second-epoch image center 16:19:04.260 -25:57:13.34
Angular distance between the image centers 0.0604 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 16:19:01.945 -25:57:34.94
Second-epoch second image center 16:19:04.260 -25:57:13.34
Angular distance between the image centers 0.01055 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/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits &> /tmp/tmp.4U2mUBGmZ5
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits &> /tmp/tmp.wqXIuXOUQH
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits &> /tmp/tmp.tKzdejBJWQ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits &> /tmp/tmp.11al58AjqL
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits
Calibrating the magnitude scale
Found non-empty wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.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_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits and wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.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_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits and wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat
Found non-empty wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits and wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat
The reference image (wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits) and catalog (wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat) found
'wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat' -> 'wcsmag.cat'
Read 8752 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 235.6487 to 253.8106 deg, Dec -31.3044 to -20.4499 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 235.6487 to 253.8106 deg, Dec -31.3044 to -20.4499 deg
Loaded 8190 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): 5578 out of 5823 total matches.
Matched with Tycho-2 5823 out of 8752 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.788280
a=0.000000 b=1.000000 c=22.788280
From vast_summary.log: estimated ref. image limiting mag.: -8.21
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.58
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.58
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
2.2 pix Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
3.2 pix fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits
3.2 pix fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits
Limiting magnitude estimates:
14.6 mag. Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
14.6 mag. Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
11.9 mag. fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits
12.1 mag. fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits
All-image limiting magnitude estimate: 11.9 (SNR ) 10.1 (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.4U2mUBGmZ5 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits' -> 'wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
WCS_IMAGE_NAME=wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
WCS-calibrated image found: wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
Checking if the catalog wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat corresponding to the image wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits alredy exist and is non-empty...
Catalog wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat corresponding to the image wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
WCS catalog name: wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=696, passed=8752
Got 8752 stars (including 8042 good ones) from the SExtractor catalog wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat
util/solve_plate_with_UCAC5 got 8752 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 931 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 8526 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 8526 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 962 matched stars entering correct_measured_positions(), 8526 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits -region wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.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.wqXIuXOUQH (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits' -> 'wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
WCS_IMAGE_NAME=wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
WCS-calibrated image found: wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
Checking if the catalog wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat corresponding to the image wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits alredy exist and is non-empty...
Catalog wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat corresponding to the image wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
WCS catalog name: wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=689, passed=8852
Got 8852 stars (including 8148 good ones) from the SExtractor catalog wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat
util/solve_plate_with_UCAC5 got 8852 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 937 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 8676 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 349 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 8673 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 960 matched stars entering correct_measured_positions(), 8672 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits -region wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.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.tKzdejBJWQ (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_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.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_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits
WCS_IMAGE_NAME=wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits
WCS-calibrated image found: wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits
Checking if the catalog wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits.cat corresponding to the image wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits.cat corresponding to the image wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits
WCS catalog name: wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=97, passed=1261
Got 1261 stars (including 1164 good ones) from the SExtractor catalog wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits.cat
util/solve_plate_with_UCAC5 got 1261 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (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 294 to 349 (Dec -31.2 to -20.5)
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 922 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.89"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 1213 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.88"
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 294 to 349 (Dec -31.2 to -20.5)
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 1215 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.98"
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 1215 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.02"
Excluding outliers - 955 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits -region wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.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.11al58AjqL (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_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.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_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits
WCS_IMAGE_NAME=wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits
WCS-calibrated image found: wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits
Checking if the catalog wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits.cat corresponding to the image wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits.cat corresponding to the image wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits
WCS catalog name: wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=72, passed=1388
Got 1388 stars (including 1314 good ones) from the SExtractor catalog wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits.cat
util/solve_plate_with_UCAC5 got 1388 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (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 293 to 349 (Dec -31.2 to -20.5)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 911 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.87"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 1319 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.89"
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 293 to 349 (Dec -31.2 to -20.5)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 1320 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.95"
Accuracy estimation diagnostic: 954 matched stars entering correct_measured_positions(), 1320 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.98"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits -region wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.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_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits'
Saving fully-calibrated image wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits'
Saving fully-calibrated image wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits'
Saving fully-calibrated image wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits'
Preparing the HTML report for the field Sco-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Sco-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits
SExtractor catalog cache: saved Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat to cache
SExtractor catalog cache: saved Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
Creating symlink local_wcs_cache/wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
Creating symlink local_wcs_cache/wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits
Creating symlink local_wcs_cache/wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.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_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits exists and is non-empty
wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits exists and is non-empty
wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits exists and is non-empty
wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits (1st reference image)
verification OK: wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
Image size: 941.6'x627.5' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 16:19:16.444 -25:59:35.75 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits (1st new image)
verification OK: wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits
Image size: 937.0'x624.4' 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: 16:19:01.945 -25:57:34.94 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 16:19:16.444 -25:59:35.75
Second-epoch image center 16:19:01.945 -25:57:34.94
Angular distance between the image centers 0.0638 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits (2nd new image)
verification OK: wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits
Image size: 937.0'x624.4' 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: 16:19:04.260 -25:57:13.34 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 16:19:16.444 -25:59:35.75
Second-epoch image center 16:19:04.260 -25:57:13.34
Angular distance between the image centers 0.0604 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 16:19:01.945 -25:57:34.94
Second-epoch second image center 16:19:04.260 -25:57:13.34
Angular distance between the image centers 0.01055 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/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits &> /tmp/tmp.9npsrqtwtl
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits &> /tmp/tmp.dhOPgAvVF6
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits &> /tmp/tmp.YY7NnrqRpv
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits &> /tmp/tmp.P484JFcZEL
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits
Calibrating the magnitude scale
Found non-empty wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.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_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits and wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.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_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits and wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat
Found non-empty wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits and wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat
The reference image (wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits) and catalog (wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat) found
'wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat' -> 'wcsmag.cat'
Read 85371 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 235.5879 to 253.8599 deg, Dec -31.3044 to -20.3796 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 235.5879 to 253.8599 deg, Dec -31.3044 to -20.3796 deg
Loaded 8263 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): 6163 out of 6991 total matches.
Matched with Tycho-2 6991 out of 85371 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.596036
a=0.000000 b=1.000000 c=22.596036
From vast_summary.log: estimated ref. image limiting mag.: -7.88
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.72
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.72
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 10 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
2.0 pix Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
3.0 pix fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits
2.9 pix fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits
Limiting magnitude estimates:
14.7 mag. Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
14.7 mag. Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
13.1 mag. fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits
13.2 mag. fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits
All-image limiting magnitude estimate: 13.1 (SNR ) 12.5 (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.9npsrqtwtl (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits' -> 'wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
WCS_IMAGE_NAME=wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
WCS-calibrated image found: wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
Checking if the catalog wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat corresponding to the image wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits alredy exist and is non-empty...
Catalog wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat corresponding to the image wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
WCS catalog name: wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=4769, passed=85367
Got 85367 stars (including 80428 good ones) from the SExtractor catalog wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat
util/solve_plate_with_UCAC5 got 85367 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 350 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 938 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 82949 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 350 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 82952 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 82952 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits -region wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.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.dhOPgAvVF6 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits' -> 'wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
WCS_IMAGE_NAME=wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
WCS-calibrated image found: wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
Checking if the catalog wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat corresponding to the image wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits alredy exist and is non-empty...
Catalog wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat corresponding to the image wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
WCS catalog name: wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=4773, passed=84610
Got 84610 stars (including 79676 good ones) from the SExtractor catalog wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat
util/solve_plate_with_UCAC5 got 84610 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 293 to 350 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 945 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 82487 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
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 293 to 350 (Dec -31.3 to -20.4)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 82488 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 82487 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits -region wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.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.YY7NnrqRpv (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_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.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_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits
WCS_IMAGE_NAME=wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits
WCS-calibrated image found: wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits
Checking if the catalog wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits.cat corresponding to the image wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits.cat corresponding to the image wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits
WCS catalog name: wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=761, passed=11973
Got 11973 stars (including 11198 good ones) from the SExtractor catalog wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits.cat
util/solve_plate_with_UCAC5 got 11973 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (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 293 to 349 (Dec -31.2 to -20.4)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 917 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.85"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 11558 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.78"
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 293 to 349 (Dec -31.2 to -20.4)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 11558 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.79"
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 11558 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.90"
Excluding outliers - 951 stars left (next iteration limit 1046)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits -region wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.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.P484JFcZEL (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_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.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_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits
WCS_IMAGE_NAME=wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits
WCS-calibrated image found: wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits
Checking if the catalog wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits.cat corresponding to the image wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits.cat corresponding to the image wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits
WCS catalog name: wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=537, passed=14328
Got 14328 stars (including 13768 good ones) from the SExtractor catalog wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits.cat
util/solve_plate_with_UCAC5 got 14328 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (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 293 to 349 (Dec -31.2 to -20.5)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 917 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.85"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 13794 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
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 293 to 349 (Dec -31.2 to -20.5)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 13790 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.73"
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 13791 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.82"
Excluding outliers - 955 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits -region wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.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_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.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_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/wcs_Sco-02-Q2b1x1_2026-02-27_05-09-40_20.00sec_-14.90C_LIGHT_0010.fits
Saving fully-calibrated image wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.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_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/wcs_Sco-02-Q2b1x1_2026-02-27_05-10-17_20.00sec_-14.90C_LIGHT_0011.fits
Saving fully-calibrated image wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.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_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-52-34_20.00sec_-4.90C_LIGHT_0000.fits
Saving fully-calibrated image wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.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_2026-04-20_CI_Sco-02-Q2b1x1_045424_TTUQ2b1x1_1263273_LB2eQE8z/wcs_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001.fits
Preparing the HTML report for the field Sco-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_local.txt__out13872.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out14211.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37662.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 4s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102149_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001
The candidate 102149_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001 did not pass the final checks
**** FOUND 16:02:42.95 -26:54:37.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102333_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001
The candidate 102333_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001 did not pass the final checks
**** FOUND 16:03:54.05 -26:48:36.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103417_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001
The candidate 103417_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001 did not pass the final checks
**** FOUND 16:36:11.64 -24:47:44.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103457_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001
The candidate 103457_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001 did not pass the final checks
**** FOUND 16:08:02.80 -26:17:28.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 79343_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001
The candidate 79343_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001 did not pass the final checks
**** FOUND 16:18:05.53 -21:49:07.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14211_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001
Preparing report for the candidate 14211_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 76483_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001
The candidate 76483_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001 did not pass the final checks
**** FOUND 16:26:39.21 -22:19:00.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37662_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001
Preparing report for the candidate 37662_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 13872_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001
Preparing report for the candidate 13872_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 48506_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001
The candidate 48506_fd_Sco-02-Q2b1x1_2026-04-20_04-53-40_20.00sec_-4.90C_LIGHT_0001 did not pass the final checks