This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4043837882501605632,2461132.9427,13.00,0.05,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
Gaia DR3 4043837882501605632 20260402.4427 13.00CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
OGLE-BLG-RRLYR-07686,2461132.9427,13.08,0.05,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
OGLE-BLG-RRLYR-07686 20260402.4427 13.08CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 4043105740840446976,2461132.9427,12.50,0.05,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
Gaia DR3 4043105740840446976 20260402.4427 12.50CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Mis V0536,2461132.9427,12.35,0.05,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
Mis V0536 20260402.4427 12.35CV 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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J175450-3412.8,2461132.9427,12.16,0.05,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
ASAS J175450-3412.8 20260402.4427 12.16CV 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: 2461098.99490872 27.02.2026 11:52:30.113 /data_ssd/NMW-TexasTech/reference_imgs/Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits
First image: 2461098.99490872 27.02.2026 11:52:30.113 /data_ssd/NMW-TexasTech/reference_imgs/Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits
Last image: 2461132.94389559 02.04.2026 10:39:02.579 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 7
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.83
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 9505
Objects passed selection criteria: 9504
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 8789.5
Average stars matched: 8556.5 (97.3491 %)
Memory usage VmPeak: 115700 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 1 15:05:04 CDT 2026
VaST build number 1.0rc88-372-gf0c1109d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-01)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 2 05:41:12 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: 2461098.99490872 27.02.2026 11:52:30.113 /data_ssd/NMW-TexasTech/reference_imgs/Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits
First image: 2461098.99490872 27.02.2026 11:52:30.113 /data_ssd/NMW-TexasTech/reference_imgs/Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits
Last image: 2461132.94389559 02.04.2026 10:39:02.579 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 147
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.42
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: 45 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): 109088
Objects passed selection criteria: 108921
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 96508.5
Average stars matched: 91619.2 (94.9339 %)
Memory usage VmPeak: 1942292 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 1 15:05:04 CDT 2026
VaST build number 1.0rc88-372-gf0c1109d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-01)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 2 05:42:58 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-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits
SExtractor catalog cache: saved Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits.cat to cache
SExtractor catalog cache: saved Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.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-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.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: 2461132.94146821
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits exists and is non-empty
Saving wcs_Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits to local_wcs_cache/
'wcs_Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits' -> 'local_wcs_cache/wcs_Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits'
wcs_Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits exists and is non-empty
Saving wcs_Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits to local_wcs_cache/
'wcs_Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits' -> 'local_wcs_cache/wcs_Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits'
wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits exists and is non-empty
Saving wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits to local_wcs_cache/
'wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits' -> 'local_wcs_cache/wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits'
wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits exists and is non-empty
Saving wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits to local_wcs_cache/
'wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits' -> 'local_wcs_cache/wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits'
The image scale is 5.88"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 17:44:23.486 -33:59:41.72
Second-epoch image center 17:44:31.409 -33:57:19.83
Angular distance between the image centers 0.05 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 17:44:23.486 -33:59:41.72
Second-epoch image center 17:44:31.391 -33:56:59.29
Angular distance between the image centers 0.05 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 17:44:31.409 -33:57:19.83
Second-epoch second image center 17:44:31.391 -33:56:59.29
Angular distance between the image centers 0.00571 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-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits &> /tmp/tmp.5bYiHIheiQ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits &> /tmp/tmp.O2BOzKg44t
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits &> /tmp/tmp.Y63wnz44e5
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits &> /tmp/tmp.pOXNR2iKJa
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits
Calibrating the magnitude scale
Found non-empty wcs_Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.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-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits and wcs_Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.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-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits and wcs_Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits.cat
Found non-empty wcs_Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits and wcs_Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits.cat
The reference image (wcs_Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits) and catalog (wcs_Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits.cat) found
'wcs_Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits.cat' -> 'wcsmag.cat'
Read 11461 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 256.0353 to 276.0310 deg, Dec -39.2725 to -28.4470 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 256.0353 to 276.0310 deg, Dec -39.2725 to -28.4470 deg
Loaded 23663 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): 8906 out of 9199 total matches.
Matched with Tycho-2 9199 out of 11461 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.562163
a=0.000000 b=1.000000 c=22.562163
From vast_summary.log: estimated ref. image limiting mag.: -8.83
Updating vast_summary.log: Estimated ref. image limiting mag.: 13.73
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 13.73
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.4 pix Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits
2.4 pix Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits
2.5 pix fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits
3.2 pix fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits
Limiting magnitude estimates:
13.7 mag. Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits
13.8 mag. Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits
13.4 mag. fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits
13.4 mag. fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits
All-image limiting magnitude estimate: 13.4 (SNR ) 10.7 (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.5bYiHIheiQ (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.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-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits' -> 'wcs_Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits
WCS_IMAGE_NAME=wcs_Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits
WCS-calibrated image found: wcs_Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits
Checking if the catalog wcs_Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits.cat corresponding to the image wcs_Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits alredy exist and is non-empty...
Catalog wcs_Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits.cat corresponding to the image wcs_Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits
WCS catalog name: wcs_Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=970, passed=11461
Got 11461 stars (including 10482 good ones) from the SExtractor catalog wcs_Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits.cat
util/solve_plate_with_UCAC5 got 11461 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 938.8'
Seting catalog search parameters based on the expected field of view 938.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013039 (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 0.010431 (37.6 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 253 to 309 (Dec -39.3 to -28.4)
Done reading UCAC5 zone files...
Matched 920 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.89"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.91"
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 253 to 309 (Dec -39.3 to -28.4)
Done reading UCAC5 zone files...
Matched 922 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.92"
Estimated accuracy of the plate solution: 1.09"
Excluding outliers - 903 stars left (next iteration limit 995)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits -region wcs_Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.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.O2BOzKg44t (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.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-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits' -> 'wcs_Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits
WCS_IMAGE_NAME=wcs_Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits
WCS-calibrated image found: wcs_Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits
Checking if the catalog wcs_Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits.cat corresponding to the image wcs_Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits alredy exist and is non-empty...
Catalog wcs_Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits.cat corresponding to the image wcs_Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits
WCS catalog name: wcs_Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1009, passed=11426
Got 11426 stars (including 10401 good ones) from the SExtractor catalog wcs_Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits.cat
util/solve_plate_with_UCAC5 got 11426 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.8'
Seting catalog search parameters based on the expected field of view 938.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013039 (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 0.010431 (37.6 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 253 to 309 (Dec -39.3 to -28.4)
Done reading UCAC5 zone files...
Matched 924 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.84"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.86"
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 253 to 309 (Dec -39.3 to -28.4)
Done reading UCAC5 zone files...
Matched 926 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.87"
Estimated accuracy of the plate solution: 0.96"
Excluding outliers - 907 stars left (next iteration limit 999)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits -region wcs_Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.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.Y63wnz44e5 (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_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.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_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits
WCS_IMAGE_NAME=wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits
WCS-calibrated image found: wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits
Checking if the catalog wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits.cat corresponding to the image wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits.cat corresponding to the image wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits
WCS catalog name: wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=856, passed=8656
Got 8656 stars (including 7790 good ones) from the SExtractor catalog wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits.cat
util/solve_plate_with_UCAC5 got 8656 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010419 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 310 (Dec -39.2 to -28.3)
Done reading UCAC5 zone files...
Matched 928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.83"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.90"
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 253 to 310 (Dec -39.2 to -28.3)
Done reading UCAC5 zone files...
Matched 928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.92"
Estimated accuracy of the plate solution: 1.03"
Excluding outliers - 912 stars left (next iteration limit 1005)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits -region wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.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.pOXNR2iKJa (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_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.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_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits
WCS_IMAGE_NAME=wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits
WCS-calibrated image found: wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits
Checking if the catalog wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits.cat corresponding to the image wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits.cat corresponding to the image wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits
WCS catalog name: wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=812, passed=9829
Got 9829 stars (including 9011 good ones) from the SExtractor catalog wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits.cat
util/solve_plate_with_UCAC5 got 9829 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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 253 to 310 (Dec -39.2 to -28.3)
Done reading UCAC5 zone files...
Matched 919 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 1.24"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 1.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 310 (Dec -39.2 to -28.3)
Done reading UCAC5 zone files...
Matched 921 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 1.32"
Estimated accuracy of the plate solution: 1.49"
Excluding outliers - 903 stars left (next iteration limit 993)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits -region wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.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-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/wcs_Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits'
Saving fully-calibrated image wcs_Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/wcs_Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits'
Saving fully-calibrated image wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits'
Saving fully-calibrated image wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits'
Preparing the HTML report for the field Sco-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20684_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
The candidate 20684_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 18:01:56.06 -35:11:34.4 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Sco-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits
SExtractor catalog cache: saved Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits.cat to cache
SExtractor catalog cache: saved Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.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-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits
Creating symlink local_wcs_cache/wcs_Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits
Creating symlink local_wcs_cache/wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits
Creating symlink local_wcs_cache/wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.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-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits exists and is non-empty
wcs_Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits exists and is non-empty
wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits exists and is non-empty
wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits exists and is non-empty
The image scale is 5.88"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 17:44:23.486 -33:59:41.72
Second-epoch image center 17:44:31.409 -33:57:19.83
Angular distance between the image centers 0.05 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 17:44:23.486 -33:59:41.72
Second-epoch image center 17:44:31.391 -33:56:59.29
Angular distance between the image centers 0.05 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 17:44:31.409 -33:57:19.83
Second-epoch second image center 17:44:31.391 -33:56:59.29
Angular distance between the image centers 0.00571 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-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits &> /tmp/tmp.3ZjZx18P7G
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits &> /tmp/tmp.CfMIEjI7Nl
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits &> /tmp/tmp.JfD8gy80b4
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits &> /tmp/tmp.Qyln4AgaOJ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits
Calibrating the magnitude scale
Found non-empty wcs_Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.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-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits and wcs_Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.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-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits and wcs_Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits.cat
Found non-empty wcs_Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits and wcs_Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits.cat
The reference image (wcs_Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits) and catalog (wcs_Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits.cat) found
'wcs_Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits.cat' -> 'wcsmag.cat'
Read 131235 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 256.0353 to 276.1068 deg, Dec -39.2831 to -28.4039 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 256.0353 to 276.1068 deg, Dec -39.2831 to -28.4039 deg
Loaded 23882 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): 17026 out of 19896 total matches.
Matched with Tycho-2 19896 out of 131235 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.258988
a=0.000000 b=1.000000 c=22.258988
From vast_summary.log: estimated ref. image limiting mag.: -8.42
Updating vast_summary.log: Estimated ref. image limiting mag.: 13.84
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 13.84
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 51 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits
2.2 pix Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits
2.3 pix fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits
2.9 pix fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits
Limiting magnitude estimates:
13.8 mag. Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits
13.8 mag. Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits
13.5 mag. fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits
13.5 mag. fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits
All-image limiting magnitude estimate: 13.5 (SNR ) 12.7 (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.3ZjZx18P7G (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.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-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits' -> 'wcs_Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits
WCS_IMAGE_NAME=wcs_Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits
WCS-calibrated image found: wcs_Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits
Checking if the catalog wcs_Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits.cat corresponding to the image wcs_Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits alredy exist and is non-empty...
Catalog wcs_Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits.cat corresponding to the image wcs_Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits
WCS catalog name: wcs_Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=11842, passed=131223
Got 131223 stars (including 119209 good ones) from the SExtractor catalog wcs_Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits.cat
util/solve_plate_with_UCAC5 got 131223 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.8'
Seting catalog search parameters based on the expected field of view 938.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013039 (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 0.010431 (37.6 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 253 to 309 (Dec -39.3 to -28.4)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.85"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.87"
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 253 to 309 (Dec -39.3 to -28.4)
Done reading UCAC5 zone files...
Matched 936 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.87"
Estimated accuracy of the plate solution: 1.00"
Excluding outliers - 924 stars left (next iteration limit 1018)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits -region wcs_Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.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.CfMIEjI7Nl (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.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-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits' -> 'wcs_Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits
WCS_IMAGE_NAME=wcs_Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits
WCS-calibrated image found: wcs_Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits
Checking if the catalog wcs_Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits.cat corresponding to the image wcs_Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits alredy exist and is non-empty...
Catalog wcs_Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits.cat corresponding to the image wcs_Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits
WCS catalog name: wcs_Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=12422, passed=135115
Got 135115 stars (including 122527 good ones) from the SExtractor catalog wcs_Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits.cat
util/solve_plate_with_UCAC5 got 135115 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.8'
Seting catalog search parameters based on the expected field of view 938.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013039 (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 0.010431 (37.6 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 253 to 310 (Dec -39.3 to -28.4)
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.81"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.82"
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 253 to 310 (Dec -39.3 to -28.4)
Done reading UCAC5 zone files...
Matched 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.82"
Estimated accuracy of the plate solution: 0.94"
Excluding outliers - 929 stars left (next iteration limit 1021)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits -region wcs_Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.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.JfD8gy80b4 (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_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.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_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits
WCS_IMAGE_NAME=wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits
WCS-calibrated image found: wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits
Checking if the catalog wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits.cat corresponding to the image wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits.cat corresponding to the image wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits
WCS catalog name: wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=8438, passed=102685
Got 102685 stars (including 94103 good ones) from the SExtractor catalog wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits.cat
util/solve_plate_with_UCAC5 got 102685 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010419 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 253 to 310 (Dec -39.2 to -28.3)
Done reading UCAC5 zone files...
Matched 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.76"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.79"
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 253 to 310 (Dec -39.2 to -28.3)
Done reading UCAC5 zone files...
Matched 939 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.79"
Estimated accuracy of the plate solution: 0.92"
Excluding outliers - 927 stars left (next iteration limit 1025)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits -region wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.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.Qyln4AgaOJ (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_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.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_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits
WCS_IMAGE_NAME=wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits
WCS-calibrated image found: wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits
Checking if the catalog wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits.cat corresponding to the image wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits alredy exist and is non-empty...
Catalog wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits.cat corresponding to the image wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits
WCS catalog name: wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=8294, passed=82349
Got 82349 stars (including 73964 good ones) from the SExtractor catalog wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits.cat
util/solve_plate_with_UCAC5 got 82349 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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 253 to 310 (Dec -39.2 to -28.3)
Done reading UCAC5 zone files...
Matched 926 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 1.12"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 1.17"
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 253 to 310 (Dec -39.2 to -28.3)
Done reading UCAC5 zone files...
Matched 927 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 1.17"
Estimated accuracy of the plate solution: 1.35"
Excluding outliers - 910 stars left (next iteration limit 999)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits -region wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.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-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.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_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/wcs_Sco-04-Q2b1x1_2026-02-27_05-52-30_20.00sec_-14.90C_LIGHT_0297.fits
Saving fully-calibrated image wcs_Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.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_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/wcs_Sco-04-Q2b1x1_2026-02-27_05-53-14_20.00sec_-15.00C_LIGHT_0298.fits
Saving fully-calibrated image wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.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_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-35-32_20.00sec_-14.90C_LIGHT_0099.fits
Saving fully-calibrated image wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.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_2026-04-02_CI_Sco-04-Q2b1x1_053945_TTUQ2b1x1_6829_cslwOV3Z/wcs_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100.fits
Preparing the HTML report for the field Sco-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out109107.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out155874.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out155906.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out155941.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out155962.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out156026.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out156039.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out156040.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out156052.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out156111.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out156115.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out156158.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out156251.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out156958.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out157339.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out56164.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out156062.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out155841.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out155847.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out156043.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out156080.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55309.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
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: 3s
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Considering the candidate 155841_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 155841_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 155847_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 155847_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 155860_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
The candidate 155860_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (16.4") between the two second-epoch detections
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Considering the candidate 155874_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
The candidate 155874_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 17:40:36.56 -36:02:21.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 4.751 4041150774804761600 265.15099733262 -36.04014668545 12.3757 11.2870 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.751#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 155906_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
The candidate 155906_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 17:40:10.12 -31:16:39.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.83, MAG_FAINT_SEARCH_LIMIT=13.81)GAIADR2_OUTPUT=# 3.637 4055176351288583168 265.04189553662 -31.27859456185 13.0478 12.5503 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.637#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 155941_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
The candidate 155941_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 17:43:01.22 -33:47:00.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.75, MAG_FAINT_SEARCH_LIMIT=13.73)GAIADR2_OUTPUT=# 4.025 4053830308543697920 265.75391093211 -33.78396478031 11.8498 10.5707 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.025#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 155962_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
The candidate 155962_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 17:53:28.69 -30:41:06.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)
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Considering the candidate 155994_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
The candidate 155994_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 17:12:27.07 -31:48:57.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 156011_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
The candidate 156011_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 18:02:25.94 -34:45:07.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 156026_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
The candidate 156026_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 18:05:20.28 -34:25:29.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)
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Considering the candidate 156037_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
The candidate 156037_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 156039_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
The candidate 156039_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 17:32:02.14 -31:09:14.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.53, MAG_FAINT_SEARCH_LIMIT=13.51)GAIADR2_OUTPUT=# 3.206 4058313361043074432 263.00994316979 -31.15409025397 12.4954 11.3287 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.206#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 156040_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
The candidate 156040_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 17:23:10.64 -30:53:03.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 4.798 4058161903315201920 260.79588644375 -30.88416460367 12.2929 11.2413 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.798#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 156043_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 156043_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 156052_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
The candidate 156052_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 17:33:55.64 -31:00:12.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 5.559 4055340006720410880 263.48102317144 -31.00482355609 12.5007 11.5481 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.559#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 156062_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
The candidate 156062_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 17:43:02.80 -35:18:16.4 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)
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Considering the candidate 156080_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 156080_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 156084_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
The candidate 156084_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 156111_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
The candidate 156111_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 17:15:09.28 -29:54:52.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 4.147 4107283719160425216 258.78864226131 -29.91559630522 12.0411 11.3150 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.147#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 156115_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
The candidate 156115_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 18:09:50.86 -32:13:48.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)
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Considering the candidate 156158_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
The candidate 156158_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 17:14:35.01 -33:07:59.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.50, MAG_FAINT_SEARCH_LIMIT=12.48)GAIADR2_OUTPUT=# 3.926 5979077780113010816 258.64571823585 -33.13222295547 11.9870 11.8415 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.926#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 156251_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
The candidate 156251_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 17:19:31.39 -30:39:47.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.47, MAG_FAINT_SEARCH_LIMIT=11.45)GAIADR2_OUTPUT=# 3.864 4058954449433106048 259.88179479592 -30.66386056804 11.0243 10.1998 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.864#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 156816_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
The candidate 156816_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 17:58:40.61 -36:04:24.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 156868_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
The candidate 156868_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 18:13:10.58 -34:02:14.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 156958_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
The candidate 156958_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 18:05:08.27 -37:25:28.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)
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Considering the candidate 156976_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
The candidate 156976_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 157003_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
The candidate 157003_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 18:01:48.73 -36:07:13.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157077_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
The candidate 157077_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 18:05:46.06 -36:23:33.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157085_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
The candidate 157085_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 17:16:51.24 -33:21:33.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157190_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
The candidate 157190_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 18:08:25.29 -29:46:59.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157242_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
The candidate 157242_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 17:57:25.83 -37:17:02.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157277_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
The candidate 157277_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 18:13:04.38 -31:57:11.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157291_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
The candidate 157291_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 18:07:04.93 -31:21:37.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157302_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
The candidate 157302_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 18:02:00.43 -36:46:54.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157339_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
The candidate 157339_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 17:59:01.92 -38:01:10.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.75, MAG_FAINT_SEARCH_LIMIT=13.73)GAIADR2_OUTPUT=# 2.004 4036994655212215808 269.75751883204 -38.01928690591 12.4911 11.3292 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.004#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 157348_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
The candidate 157348_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 18:07:43.30 -31:01:53.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157565_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
The candidate 157565_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 17:56:20.88 -37:50:16.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157616_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
The candidate 157616_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
Rejecting candidate due to large distance (21.6") between the two second-epoch detections
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Considering the candidate 157639_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
The candidate 157639_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 18:12:24.72 -33:50:20.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157664_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
The candidate 157664_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 18:00:12.30 -33:51:03.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157812_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
The candidate 157812_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 17:57:37.92 -37:51:06.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157836_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
The candidate 157836_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 17:11:51.24 -33:34:06.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157853_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
The candidate 157853_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 18:06:00.23 -31:36:53.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 157885_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
The candidate 157885_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 18:13:45.53 -34:34:18.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 158571_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
The candidate 158571_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 17:52:12.12 -34:20:57.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 109107_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
The candidate 109107_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 18:11:52.51 -30:10:06.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.82, MAG_FAINT_SEARCH_LIMIT=12.80)
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Considering the candidate 55309_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
Preparing report for the candidate 55309_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
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Considering the candidate 126669_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
The candidate 126669_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 18:10:54.38 -31:55:21.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 56164_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
The candidate 56164_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 18:08:25.17 -34:03:32.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 1.315 4039555108559297024 272.10518051915 -34.05931887156 12.9274 11.4566 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.315#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 141435_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
The candidate 141435_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks
**** FOUND 17:37:31.67 -32:55:10.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 90763_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100
The candidate 90763_fd_Sco-04-Q2b1x1_2026-04-02_05-39-02_20.00sec_-15.00C_LIGHT_0100 did not pass the final checks