This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.2088* 10 34 26.98 +01 30 45.9 11.8 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461139.7088,11.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260409.2088 11.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.2088* 10 02 50.85 +00 04 22.2 13.4 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.7088,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.2088 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.2088* 10 00 17.97 +01 03 06.1 13.4 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461139.7088,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260409.2088 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.2088* 10 41 57.67 +00 51 14.4 13.5 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461139.7088,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260409.2088 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 04 09.2088* 10 01 45.89 -02 13 16.1 10.9 U Sex 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VW Sex,2461139.7088,10.88,0.05,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
VW Sex 20260409.2088 10.88CV 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: 2461058.90489140 18.01.2026 09:42:52.617 /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
First image: 2461058.90489140 18.01.2026 09:42:52.617 /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
Last image: 2461139.70900510 09.04.2026 05:00:48.041 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 11
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.70
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): 5701
Objects passed selection criteria: 5697
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 5379.5
Average stars matched: 5250.5 (97.602 %)
Memory usage VmPeak: 112188 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 9 01:17:47 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: 2461058.90489140 18.01.2026 09:42:52.617 /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
First image: 2461058.90489140 18.01.2026 09:42:52.617 /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
Last image: 2461139.70900510 09.04.2026 05:00:48.041 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 70
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.41
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 14 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 29677
Objects passed selection criteria: 29625
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 26262
Average stars matched: 25684.2 (97.8001 %)
Memory usage VmPeak: 135380 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Apr 8 18:56:33 CDT 2026
VaST build number 1.0rc89-5-g00c52b5f
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-08)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Apr 9 01:18:44 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/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits
SExtractor catalog cache: saved Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat to cache
SExtractor catalog cache: saved Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.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/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.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: 2461139.70850777
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_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits exists and is non-empty
Saving wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits to local_wcs_cache/
'wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits' -> 'local_wcs_cache/wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits'
wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits exists and is non-empty
Saving wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits to local_wcs_cache/
'wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits' -> 'local_wcs_cache/wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits'
wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits exists and is non-empty
Saving wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits to local_wcs_cache/
'wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits' -> 'local_wcs_cache/wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits'
wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits exists and is non-empty
Saving wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits to local_wcs_cache/
'wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits' -> 'local_wcs_cache/wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 10:17:03.829 -01:59:47.05
Second-epoch image center 10:17:09.010 -01:59:59.66
Angular distance between the image centers 0.0219 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 10:17:03.829 -01:59:47.05
Second-epoch image center 10:17:09.040 -02:00:03.23
Angular distance between the image centers 0.0222 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 10:17:09.010 -01:59:59.66
Second-epoch second image center 10:17:09.040 -02:00:03.23
Angular distance between the image centers 0.00100 deg.
###################################
ERROR: no shift applied between second-epoch images! The distance between image centers is 0.00100 deg. (min. required shift: 0.00164 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/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits &> /tmp/tmp.T6RdeJxz0w
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits &> /tmp/tmp.5sQBeuv3zC
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits &> /tmp/tmp.ZTNrcQnVNB
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits &> /tmp/tmp.aM2x4zmRrK
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits
Calibrating the magnitude scale
Found non-empty wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.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_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits and wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.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_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits and wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat
Found non-empty wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits and wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat
The reference image (wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits) and catalog (wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat) found
'wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat' -> 'wcsmag.cat'
Read 7808 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 146.3749 to 162.2183 deg, Dec -7.3004 to +3.3307 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 146.3749 to 162.2183 deg, Dec -7.3004 to 3.3307 deg
Loaded 4796 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): 4045 out of 4187 total matches.
Matched with Tycho-2 4187 out of 7808 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.873667
a=0.000000 b=1.000000 c=22.873667
From vast_summary.log: estimated ref. image limiting mag.: -7.70
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.17
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.17
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 7 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
2.3 pix Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
4.3 pix fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits
4.3 pix fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits
Limiting magnitude estimates:
15.2 mag. Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
15.2 mag. Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
14.5 mag. fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits
14.5 mag. fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 12.0 (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.T6RdeJxz0w (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits' -> 'wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
WCS_IMAGE_NAME=wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
WCS-calibrated image found: wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
Checking if the catalog wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat corresponding to the image wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits alredy exist and is non-empty...
Catalog wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat corresponding to the image wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
WCS catalog name: wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=466, passed=7808
Got 7808 stars (including 7337 good ones) from the SExtractor catalog wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat
util/solve_plate_with_UCAC5 got 7808 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 916 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 7570 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 7573 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 7573 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 931 stars left (next iteration limit 1024)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits -region wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.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.5sQBeuv3zC (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits' -> 'wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
WCS_IMAGE_NAME=wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
WCS-calibrated image found: wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
Checking if the catalog wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat corresponding to the image wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits alredy exist and is non-empty...
Catalog wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat corresponding to the image wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
WCS catalog name: wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=461, passed=7862
Got 7862 stars (including 7394 good ones) from the SExtractor catalog wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat
util/solve_plate_with_UCAC5 got 7862 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 917 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 7613 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 7616 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 7616 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 934 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits -region wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.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.ZTNrcQnVNB (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_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.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_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits
WCS_IMAGE_NAME=wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits
WCS-calibrated image found: wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits
Checking if the catalog wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits.cat corresponding to the image wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits alredy exist and is non-empty...
Catalog wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits.cat corresponding to the image wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits
WCS catalog name: wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=899, passed=6431
Got 6431 stars (including 5531 good ones) from the SExtractor catalog wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits.cat
util/solve_plate_with_UCAC5 got 6431 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.6'
Seting catalog search parameters based on the expected field of view 936.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013008 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010407 (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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 925 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 924 matched stars entering correct_measured_positions(), 909 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 924 matched stars entering correct_measured_positions(), 6082 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 925 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 924 matched stars entering correct_measured_positions(), 6081 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Accuracy estimation diagnostic: 924 matched stars entering correct_measured_positions(), 6081 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
Excluding outliers - 924 stars left (next iteration limit 1016)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits -region wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.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.aM2x4zmRrK (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_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.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_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits
WCS_IMAGE_NAME=wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits
WCS-calibrated image found: wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits
Checking if the catalog wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits.cat corresponding to the image wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits alredy exist and is non-empty...
Catalog wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits.cat corresponding to the image wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits
WCS catalog name: wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=923, passed=6460
Got 6460 stars (including 5535 good ones) from the SExtractor catalog wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits.cat
util/solve_plate_with_UCAC5 got 6460 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.6'
Seting catalog search parameters based on the expected field of view 936.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013008 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010407 (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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 925 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 924 matched stars entering correct_measured_positions(), 911 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 924 matched stars entering correct_measured_positions(), 6131 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.71"
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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 925 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 924 matched stars entering correct_measured_positions(), 6133 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.72"
Accuracy estimation diagnostic: 924 matched stars entering correct_measured_positions(), 6133 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.78"
Excluding outliers - 924 stars left (next iteration limit 1016)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits -region wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.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_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits'
Saving fully-calibrated image wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits'
Saving fully-calibrated image wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits'
Saving fully-calibrated image wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits'
Preparing the HTML report for the field Sex-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20299.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20304.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20306.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20308.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out20296.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
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 20294_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167
The candidate 20294_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167 did not pass the final checks
**** FOUND 10:25:43.88 +01:28:07.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20296_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167
Preparing report for the candidate 20296_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20299_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167
The candidate 20299_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167 did not pass the final checks
**** FOUND 10:35:55.39 -02:01:37.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.17, MAG_FAINT_SEARCH_LIMIT=13.15)GAIADR2_OUTPUT=# 0.614 3781772374039566208 158.98092412039 -02.02730202849 12.2677 11.8093 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.614#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20304_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167
The candidate 20304_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167 did not pass the final checks
**** FOUND 10:37:40.17 -00:28:30.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 0.121 3806720189794731008 159.41735497931 -00.47516737408 12.2847 11.5823 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.121#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20306_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167
The candidate 20306_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167 did not pass the final checks
**** FOUND 10:36:34.20 -00:16:16.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 0.285 3806786057413228032 159.14250600587 -00.27124573045 12.4735 12.0059 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.285#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20308_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167
The candidate 20308_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167 did not pass the final checks
**** FOUND 10:31:50.08 -00:51:28.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.33, MAG_FAINT_SEARCH_LIMIT=13.31)GAIADR2_OUTPUT=# 0.191 3782730877596355200 157.95871798354 -00.85795754084 12.2755 11.6087 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.191#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02522_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167
The candidate 02522_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167 did not pass the final checks
**** FOUND 10:34:55.95 -00:20:34.0 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 7s
Prepared the HTML report for the field Sex-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
10:34:26.98 +01:30:45.9
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/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits
SExtractor catalog cache: saved Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat to cache
SExtractor catalog cache: saved Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
Creating symlink local_wcs_cache/wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
Creating symlink local_wcs_cache/wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits
Creating symlink local_wcs_cache/wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.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_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits exists and is non-empty
wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits exists and is non-empty
wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits exists and is non-empty
wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 10:17:03.829 -01:59:47.05
Second-epoch image center 10:17:09.010 -01:59:59.66
Angular distance between the image centers 0.0219 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 10:17:03.829 -01:59:47.05
Second-epoch image center 10:17:09.040 -02:00:03.23
Angular distance between the image centers 0.0222 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 10:17:09.010 -01:59:59.66
Second-epoch second image center 10:17:09.040 -02:00:03.23
Angular distance between the image centers 0.00100 deg.
###################################
ERROR: no shift applied between second-epoch images! The distance between image centers is 0.00100 deg. (min. required shift: 0.00164 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/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits &> /tmp/tmp.qzpkvh8Ris
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits &> /tmp/tmp.GrOZRN7vXC
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits &> /tmp/tmp.qtaLFv48hA
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits &> /tmp/tmp.dz5d3q6dWY
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits
Calibrating the magnitude scale
Found non-empty wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.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_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits and wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.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_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits and wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat
Found non-empty wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits and wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat
The reference image (wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits) and catalog (wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat) found
'wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat' -> 'wcsmag.cat'
Read 40923 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 146.3591 to 162.2194 deg, Dec -7.3040 to +3.3307 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 146.3591 to 162.2194 deg, Dec -7.3040 to 3.3307 deg
Loaded 4799 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): 3845 out of 4239 total matches.
Matched with Tycho-2 4239 out of 40923 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.755743
a=0.000000 b=1.000000 c=22.755743
From vast_summary.log: estimated ref. image limiting mag.: -7.41
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.35
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.35
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 30 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
2.3 pix Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
3.8 pix fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits
3.8 pix fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits
Limiting magnitude estimates:
15.3 mag. Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
15.3 mag. Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
14.8 mag. fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits
14.8 mag. fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 14.1 (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.qzpkvh8Ris (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits' -> 'wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
WCS_IMAGE_NAME=wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
WCS-calibrated image found: wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
Checking if the catalog wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat corresponding to the image wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits alredy exist and is non-empty...
Catalog wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat corresponding to the image wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
WCS catalog name: wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=1914, passed=40911
Got 40911 stars (including 38933 good ones) from the SExtractor catalog wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat
util/solve_plate_with_UCAC5 got 40911 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 914 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 39819 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 39821 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 39821 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
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_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits -region wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.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.GrOZRN7vXC (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits' -> 'wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
WCS_IMAGE_NAME=wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
WCS-calibrated image found: wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
Checking if the catalog wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat corresponding to the image wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits alredy exist and is non-empty...
Catalog wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat corresponding to the image wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
WCS catalog name: wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=1902, passed=40634
Got 40634 stars (including 38663 good ones) from the SExtractor catalog wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat
util/solve_plate_with_UCAC5 got 40634 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 916 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 39578 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 931 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 39579 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 39579 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 931 stars left (next iteration limit 1024)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits -region wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.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.qtaLFv48hA (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_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.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_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits
WCS_IMAGE_NAME=wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits
WCS-calibrated image found: wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits
Checking if the catalog wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits.cat corresponding to the image wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits alredy exist and is non-empty...
Catalog wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits.cat corresponding to the image wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits
WCS catalog name: wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=3994, passed=26348
Got 26348 stars (including 22343 good ones) from the SExtractor catalog wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits.cat
util/solve_plate_with_UCAC5 got 26348 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.6'
Seting catalog search parameters based on the expected field of view 936.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013008 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010407 (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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 914 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 913 matched stars entering correct_measured_positions(), 901 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 913 matched stars entering correct_measured_positions(), 25048 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 914 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 913 matched stars entering correct_measured_positions(), 25049 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Accuracy estimation diagnostic: 913 matched stars entering correct_measured_positions(), 25049 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.74"
Excluding outliers - 913 stars left (next iteration limit 1004)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits -region wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.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.dz5d3q6dWY (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_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.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_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits
WCS_IMAGE_NAME=wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits
WCS-calibrated image found: wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits
Checking if the catalog wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits.cat corresponding to the image wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits alredy exist and is non-empty...
Catalog wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits.cat corresponding to the image wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits
WCS catalog name: wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=3996, passed=26505
Got 26505 stars (including 22498 good ones) from the SExtractor catalog wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits.cat
util/solve_plate_with_UCAC5 got 26505 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.6'
Seting catalog search parameters based on the expected field of view 936.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013008 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010407 (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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 915 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 914 matched stars entering correct_measured_positions(), 902 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.70"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 914 matched stars entering correct_measured_positions(), 25147 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
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 413 to 468 (Dec -7.3 to 3.3)
Done reading UCAC5 zone files...
Matched 915 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 914 matched stars entering correct_measured_positions(), 25146 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Accuracy estimation diagnostic: 914 matched stars entering correct_measured_positions(), 25145 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
Excluding outliers - 914 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_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits -region wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.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_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.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_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/wcs_Sex-02-Q2b1x1_2026-01-18_03-42-52_20.00sec_-14.90C_LIGHT_0453.fits
Saving fully-calibrated image wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.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_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/wcs_Sex-02-Q2b1x1_2026-01-18_03-43-31_20.00sec_-15.00C_LIGHT_0454.fits
Saving fully-calibrated image wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.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_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-05_20.00sec_-4.90C_LIGHT_0166.fits
Saving fully-calibrated image wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.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_2026-04-09_CI_Sex-02-Q2b1x1_011531_TTUQ2b1x1_19621_e3ulG3gf/wcs_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167.fits
Preparing the HTML report for the field Sex-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out52068.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52071.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52078.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out52080.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out20091.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52070.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52073.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52135.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 16s
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
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52068_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167
The candidate 52068_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167 did not pass the final checks
**** FOUND 10:02:06.05 +01:54:33.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)GAIADR2_OUTPUT=# 2.764 3836049082645085440 150.52446959805 +01.90940538512 13.2755 12.6113 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.764#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52070_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167
Preparing report for the candidate 52070_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52071_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167
The candidate 52071_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167 did not pass the final checks
**** FOUND 10:02:19.41 -06:05:44.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 1.208 3773448727419844608 150.58120721994 -06.09583660455 13.1315 12.6510 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.208#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52073_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167
Preparing report for the candidate 52073_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52078_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167
The candidate 52078_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167 did not pass the final checks
**** FOUND 10:43:37.65 +02:20:20.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 3.070 3809282502859140992 160.90771635138 +02.33885709650 13.4130 12.9115 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.070#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52080_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167
The candidate 52080_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167 did not pass the final checks
**** FOUND 10:01:21.04 -06:00:58.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 0.967 3821491544397985280 150.33789226905 -06.01601876704 12.7803 12.2705 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.967#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52092_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167
The candidate 52092_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167 did not pass the final checks
**** FOUND 10:25:43.88 +01:28:07.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52093_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167
The candidate 52093_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52096_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167
The candidate 52096_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167 did not pass the final checks
**** FOUND 10:34:26.97 +01:30:45.9 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52100_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167
The candidate 52100_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52108_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167
The candidate 52108_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52110_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167
The candidate 52110_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52114_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167
The candidate 52114_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167 did not pass the final checks
**** FOUND 10:34:35.92 +01:46:35.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52135_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167
Preparing report for the candidate 52135_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52137_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167
The candidate 52137_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167 did not pass the final checks
**** FOUND 10:26:49.70 -00:07:33.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52138_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167
The candidate 52138_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52139_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167
The candidate 52139_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167 did not pass the final checks
**** FOUND 10:41:13.08 -00:17:30.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52152_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167
The candidate 52152_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167 did not pass the final checks
**** FOUND 10:27:39.29 -00:56:39.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52156_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167
The candidate 52156_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52159_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167
The candidate 52159_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167 did not pass the final checks
**** FOUND 10:18:18.80 -01:13:37.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52163_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167
The candidate 52163_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52167_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167
The candidate 52167_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167 did not pass the final checks
**** FOUND 10:18:36.21 +01:34:17.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52168_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167
The candidate 52168_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167 did not pass the final checks
**** FOUND 10:14:57.79 +00:50:12.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52169_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167
The candidate 52169_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52170_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167
The candidate 52170_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52172_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167
The candidate 52172_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52179_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167
The candidate 52179_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52182_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167
The candidate 52182_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12839_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167
The candidate 12839_fd_Sex-02-Q2b1x1_2026-04-09_00-00-48_20.00sec_-4.90C_LIGHT_0167 did not pass the final checks