This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461147.8252,11.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260417.3252 11.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461147.8252,11.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260417.3252 11.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461147.8252,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260417.3252 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461147.8252,12.44,0.05,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
VARIABLE_NAME 20260417.3252 12.44CV 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461147.8252,14.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260417.3252 14.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461098.92002373 27.02.2026 10:04:40.050 /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
First image: 2461098.92002373 27.02.2026 10:04:40.050 /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
Last image: 2461147.82542069 17.04.2026 07:48:26.348 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 6
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.28
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): 5463
Objects passed selection criteria: 5462
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: 5192
Average stars matched: 4988.5 (96.0805 %)
Memory usage VmPeak: 111748 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Apr 17 02:51:41 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461098.92002373 27.02.2026 10:04:40.050 /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
First image: 2461098.92002373 27.02.2026 10:04:40.050 /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
Last image: 2461147.82542069 17.04.2026 07:48:26.348 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.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.: -7.97
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: 20 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): 34912
Objects passed selection criteria: 34850
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: 33061.5
Average stars matched: 31768.2 (96.0884 %)
Memory usage VmPeak: 137576 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Apr 17 02:53:00 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/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits
SExtractor catalog cache: saved Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat to cache
SExtractor catalog cache: saved Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.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/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461147.82490534
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_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits exists and is non-empty
Saving wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits to local_wcs_cache/
'wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits' -> 'local_wcs_cache/wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits'
wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits exists and is non-empty
Saving wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits to local_wcs_cache/
'wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits' -> 'local_wcs_cache/wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits'
wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits exists and is non-empty
Saving wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits to local_wcs_cache/
'wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits' -> 'local_wcs_cache/wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits'
wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits exists and is non-empty
Saving wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits to local_wcs_cache/
'wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits' -> 'local_wcs_cache/wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits (1st reference image)
verification OK: wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
Image size: 937.4'x624.5' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 15:07:04.132 -18:01:06.94 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits (1st new image)
verification OK: wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits
Image size: 937.0'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 15:06:24.090 -17:59:29.63 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 15:07:04.132 -18:01:06.94
Second-epoch image center 15:06:24.090 -17:59:29.63
Angular distance between the image centers 0.1610 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits (2nd new image)
verification OK: wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits
Image size: 937.0'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 15:06:24.219 -17:59:47.72 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 15:07:04.132 -18:01:06.94
Second-epoch image center 15:06:24.219 -17:59:47.72
Angular distance between the image centers 0.1597 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 15:06:24.090 -17:59:29.63
Second-epoch second image center 15:06:24.219 -17:59:47.72
Angular distance between the image centers 0.00505 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/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits &> /tmp/tmp.ASkHYldWSt
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits &> /tmp/tmp.AQBPhTc5BQ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits &> /tmp/tmp.uP34dyy5P2
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits &> /tmp/tmp.hxNDpA29Pv
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits
Calibrating the magnitude scale
Found non-empty wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.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_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits and wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.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_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits and wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat
Found non-empty wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits and wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat
The reference image (wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits) and catalog (wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat) found
'wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat' -> 'wcsmag.cat'
Read 6705 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 218.3309 to 235.1834 deg, Dec -23.2849 to -12.5918 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 218.3309 to 235.1834 deg, Dec -23.2849 to -12.5918 deg
Loaded 6143 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): 4648 out of 4760 total matches.
Matched with Tycho-2 4760 out of 6705 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.861505
a=0.000000 b=1.000000 c=22.861505
From vast_summary.log: estimated ref. image limiting mag.: -8.28
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.58
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.58
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.4 pix Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
2.4 pix Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
3.0 pix fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits
3.0 pix fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits
Limiting magnitude estimates:
14.6 mag. Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
14.6 mag. Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
14.5 mag. fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits
14.5 mag. fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 11.7 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.ASkHYldWSt (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits' -> 'wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
WCS_IMAGE_NAME=wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
WCS-calibrated image found: wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
Checking if the catalog wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat corresponding to the image wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits alredy exist and is non-empty...
Catalog wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat corresponding to the image wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
WCS catalog name: wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=403, passed=6705
Got 6705 stars (including 6294 good ones) from the SExtractor catalog wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat
util/solve_plate_with_UCAC5 got 6705 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (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 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 943 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 6630 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
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 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 6630 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 6630 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits -region wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.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.AQBPhTc5BQ (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits' -> 'wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
WCS_IMAGE_NAME=wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
WCS-calibrated image found: wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
Checking if the catalog wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat corresponding to the image wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits alredy exist and is non-empty...
Catalog wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat corresponding to the image wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
WCS catalog name: wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=425, passed=6649
Got 6649 stars (including 6218 good ones) from the SExtractor catalog wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat
util/solve_plate_with_UCAC5 got 6649 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (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 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 944 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 6582 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 6580 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 6580 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits -region wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.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.uP34dyy5P2 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits
WCS_IMAGE_NAME=wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits
WCS-calibrated image found: wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits
Checking if the catalog wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits.cat corresponding to the image wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits.cat corresponding to the image wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits
WCS catalog name: wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=456, passed=6859
Got 6859 stars (including 6400 good ones) from the SExtractor catalog wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits.cat
util/solve_plate_with_UCAC5 got 6859 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 6795 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
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 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 6798 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 6798 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Excluding outliers - 959 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits -region wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.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.hxNDpA29Pv (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits
WCS_IMAGE_NAME=wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits
WCS-calibrated image found: wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits
Checking if the catalog wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits.cat corresponding to the image wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits.cat corresponding to the image wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits
WCS catalog name: wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=511, passed=6920
Got 6920 stars (including 6405 good ones) from the SExtractor catalog wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits.cat
util/solve_plate_with_UCAC5 got 6920 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 6849 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
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 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 6850 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.53"
Accuracy estimation diagnostic: 959 matched stars entering correct_measured_positions(), 6850 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.57"
Excluding outliers - 959 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits -region wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.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_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits'
Saving fully-calibrated image wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits'
Saving fully-calibrated image wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits'
Saving fully-calibrated image wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits'
Preparing the HTML report for the field Lib-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20352.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out20303.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20331.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20252_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270
The candidate 20252_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270 did not pass the final checks
**** FOUND 15:17:57.89 -13:57:48.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20303_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270
Preparing report for the candidate 20303_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20331_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270
Preparing report for the candidate 20331_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20352_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270
The candidate 20352_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270 did not pass the final checks
**** FOUND 14:55:28.94 -16:03:52.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.81, MAG_FAINT_SEARCH_LIMIT=12.79)GAIADR2_OUTPUT=# 0.790 6306704349377967360 223.87047474915 -16.06477625718 11.7679 11.4362 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.790#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01970_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270
The candidate 01970_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270 did not pass the final checks
**** FOUND 14:42:46.39 -20:12:36.2 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 10s
Prepared the HTML report for the field Lib-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
14:58:34.62 -14:25:40.5
15:10:57.49 -21:07:10.4
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/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits
SExtractor catalog cache: saved Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat to cache
SExtractor catalog cache: saved Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
Creating symlink local_wcs_cache/wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
Creating symlink local_wcs_cache/wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits
Creating symlink local_wcs_cache/wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.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_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits exists and is non-empty
wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits exists and is non-empty
wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits exists and is non-empty
wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits (1st reference image)
verification OK: wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
Image size: 937.4'x624.5' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.87"/pix along the Y axis
Image center: 15:07:04.132 -18:01:06.94 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits (1st new image)
verification OK: wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits
Image size: 937.0'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 15:06:24.090 -17:59:29.63 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 15:07:04.132 -18:01:06.94
Second-epoch image center 15:06:24.090 -17:59:29.63
Angular distance between the image centers 0.1610 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits (2nd new image)
verification OK: wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits
Image size: 937.0'x624.3' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 15:06:24.219 -17:59:47.72 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 15:07:04.132 -18:01:06.94
Second-epoch image center 15:06:24.219 -17:59:47.72
Angular distance between the image centers 0.1597 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 15:06:24.090 -17:59:29.63
Second-epoch second image center 15:06:24.219 -17:59:47.72
Angular distance between the image centers 0.00505 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/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits &> /tmp/tmp.pXRfFWFFdE
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits &> /tmp/tmp.0ttCvgnbO1
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits &> /tmp/tmp.CuTf0L6CXO
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits &> /tmp/tmp.ZgWaRLYI98
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits
Calibrating the magnitude scale
Found non-empty wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.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_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits and wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.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_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits and wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat
Found non-empty wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits and wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat
The reference image (wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits) and catalog (wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat) found
'wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat' -> 'wcsmag.cat'
Read 42407 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 218.2429 to 235.1834 deg, Dec -23.2935 to -12.5730 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 218.2429 to 235.1834 deg, Dec -23.2935 to -12.5730 deg
Loaded 6189 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): 4998 out of 5340 total matches.
Matched with Tycho-2 5340 out of 42407 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.687465
a=0.000000 b=1.000000 c=22.687465
From vast_summary.log: estimated ref. image limiting mag.: -7.97
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.72
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.72
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 37 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.3 pix Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
2.3 pix Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
2.6 pix fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits
2.6 pix fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits
Limiting magnitude estimates:
14.7 mag. Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
14.7 mag. Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
14.6 mag. fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits
14.6 mag. fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 14.0 (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.pXRfFWFFdE (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits' -> 'wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
WCS_IMAGE_NAME=wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
WCS-calibrated image found: wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
Checking if the catalog wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat corresponding to the image wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits alredy exist and is non-empty...
Catalog wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat corresponding to the image wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
WCS catalog name: wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=1940, passed=42401
Got 42401 stars (including 40414 good ones) from the SExtractor catalog wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat
util/solve_plate_with_UCAC5 got 42401 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (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 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 939 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 42016 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
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 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 42016 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 42016 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 955 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits -region wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.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.0ttCvgnbO1 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits' -> 'wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
WCS_IMAGE_NAME=wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
WCS-calibrated image found: wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
Checking if the catalog wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat corresponding to the image wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits alredy exist and is non-empty...
Catalog wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat corresponding to the image wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
WCS catalog name: wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=1927, passed=42823
Got 42823 stars (including 40848 good ones) from the SExtractor catalog wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat
util/solve_plate_with_UCAC5 got 42823 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010416 (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 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 945 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 42414 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
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 333 to 389 (Dec -23.3 to -12.6)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 42413 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.48"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 42413 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits -region wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.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.CuTf0L6CXO (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits
WCS_IMAGE_NAME=wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits
WCS-calibrated image found: wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits
Checking if the catalog wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits.cat corresponding to the image wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits.cat corresponding to the image wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits
WCS catalog name: wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=2844, passed=37836
Got 37836 stars (including 34955 good ones) from the SExtractor catalog wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits.cat
util/solve_plate_with_UCAC5 got 37836 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 37339 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 37339 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.50"
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 37339 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 957 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits -region wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.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.ZgWaRLYI98 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits
WCS_IMAGE_NAME=wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits
WCS-calibrated image found: wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits
Checking if the catalog wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits.cat corresponding to the image wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits alredy exist and is non-empty...
Catalog wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits.cat corresponding to the image wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits
WCS catalog name: wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=1, no_mag_err=0, low_SNR=12, blended=3099, passed=38582
Got 38582 stars (including 35451 good ones) from the SExtractor catalog wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits.cat
util/solve_plate_with_UCAC5 got 38582 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.54"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 38017 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
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 333 to 389 (Dec -23.3 to -12.5)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 38018 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.52"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 38018 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits -region wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.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_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/wcs_Lib-03-Q2b1x1_2026-02-27_04-04-40_20.00sec_-15.00C_LIGHT_0225.fits
Saving fully-calibrated image wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/wcs_Lib-03-Q2b1x1_2026-02-27_04-05-21_20.00sec_-15.00C_LIGHT_0226.fits
Saving fully-calibrated image wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-47-41_20.00sec_-4.90C_LIGHT_0269.fits
Saving fully-calibrated image wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-17_CI_Lib-03-Q2b1x1_024914_TTUQ2b1x1_1286073_sOSPxgSV/wcs_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270.fits
Preparing the HTML report for the field Lib-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out53024.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53578.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53579.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53599.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53667.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out53677.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out53601.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out53150.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53203.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out53587.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: 3s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53024_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270
The candidate 53024_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270 did not pass the final checks
**** FOUND 14:49:43.66 -18:39:33.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.11, MAG_FAINT_SEARCH_LIMIT=15.09)GAIADR2_OUTPUT=# 1.786 6282026223209409792 222.43227339563 -18.65955772862 14.3643 13.8199 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.786#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53026_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270
The candidate 53026_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270 did not pass the final checks
**** FOUND 15:14:16.11 -15:35:02.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 53027_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270
The candidate 53027_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270 did not pass the final checks
**** FOUND 14:40:46.29 -14:14:06.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53036_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270
The candidate 53036_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270 did not pass the final checks
**** FOUND 14:38:25.29 -15:04:53.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53039_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270
The candidate 53039_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270 did not pass the final checks
**** FOUND 14:47:58.83 -17:05:54.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53086_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270
The candidate 53086_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270 did not pass the final checks
Rejecting candidate due to large distance (18.0") between the two second-epoch detections
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Considering the candidate 53089_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270
The candidate 53089_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270 did not pass the final checks
**** FOUND 14:58:34.62 -14:25:40.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53119_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270
The candidate 53119_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
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Considering the candidate 53126_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270
The candidate 53126_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270 did not pass the final checks
**** FOUND 15:10:57.48 -21:07:10.3 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 53150_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270
Preparing report for the candidate 53150_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270
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Considering the candidate 53179_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270
The candidate 53179_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270 did not pass the final checks
Rejecting candidate due to large distance (18.1") between the two second-epoch detections
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Considering the candidate 53190_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270
The candidate 53190_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270 did not pass the final checks
**** FOUND 14:50:34.84 -16:00:52.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 53203_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270
Preparing report for the candidate 53203_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270
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Considering the candidate 53205_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270
The candidate 53205_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
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Considering the candidate 53288_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270
The candidate 53288_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 53408_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270
The candidate 53408_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
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Considering the candidate 53455_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270
The candidate 53455_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
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Considering the candidate 53459_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270
The candidate 53459_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270 did not pass the final checks
**** FOUND 14:57:03.16 -16:18:29.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53480_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270
The candidate 53480_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270 did not pass the final checks
**** FOUND 14:42:14.81 -18:23:57.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53506_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270
The candidate 53506_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270 did not pass the final checks
**** FOUND 14:39:44.95 -13:59:53.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53534_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270
The candidate 53534_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270 did not pass the final checks
**** FOUND 15:11:53.69 -17:43:25.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53542_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270
The candidate 53542_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270 did not pass the final checks
**** FOUND 14:47:25.09 -21:33:19.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53566_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270
The candidate 53566_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270 did not pass the final checks
**** FOUND 14:47:38.05 -16:22:25.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53573_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270
The candidate 53573_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270 did not pass the final checks
**** FOUND 14:51:30.29 -13:57:44.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53578_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270
The candidate 53578_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270 did not pass the final checks
**** FOUND 14:38:49.55 -15:30:02.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 0.250 6286706706769728768 219.70640866074 -15.50069955835 14.2705 13.6460 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.250#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53579_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270
The candidate 53579_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270 did not pass the final checks
**** FOUND 14:43:55.74 -16:43:02.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.30, MAG_FAINT_SEARCH_LIMIT=15.28)GAIADR2_OUTPUT=# 1.691 6285768170516244224 220.98193885268 -16.71766860361 14.3099 13.7570 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.691#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53587_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270
Preparing report for the candidate 53587_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270
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Considering the candidate 53595_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270
The candidate 53595_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270 did not pass the final checks
**** FOUND 15:18:10.13 -21:52:16.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53599_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270
The candidate 53599_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270 did not pass the final checks
**** FOUND 14:47:58.51 -14:53:37.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 0.761 6310088817966981504 221.99360557324 -14.89352770029 14.2354 13.6701 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.761#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53601_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270
The candidate 53601_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270 did not pass the final checks
**** FOUND 14:55:12.93 -19:39:50.8 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)
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Considering the candidate 53625_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270
The candidate 53625_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270 did not pass the final checks
**** FOUND 14:39:36.82 -20:45:52.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53644_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270
The candidate 53644_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270 did not pass the final checks
**** FOUND 15:00:36.52 -17:27:55.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53657_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270
The candidate 53657_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
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Considering the candidate 53667_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270
The candidate 53667_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270 did not pass the final checks
**** FOUND 15:04:04.90 -18:01:18.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)GAIADR2_OUTPUT=# 0.845 6305248733421919104 226.02020249663 -18.02157786510 14.3206 13.8037 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.845#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53677_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270
The candidate 53677_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270 did not pass the final checks
**** FOUND 14:52:28.91 -18:48:42.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)GAIADR2_OUTPUT=# 0.308 6281346553224980480 223.12043930173 -18.81194483082 14.3324 13.7295 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.308#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 10485_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270
The candidate 10485_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270 did not pass the final checks
**** FOUND 14:42:46.39 -20:12:36.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23565_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270
The candidate 23565_fd_Lib-03-Q2b1x1_2026-04-17_02-48-26_20.00sec_-4.90C_LIGHT_0270 did not pass the final checks