This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461124.7539,12.99,0.05,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 20260325.2539 12.99CV 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
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:36:53.87 +15:56:19.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20_00sec_-15_00C_LIGHT_0235_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20_00sec_-15_00C_LIGHT_0029_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20_00sec_-15_00C_LIGHT_0235_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20_00sec_-15_00C_LIGHT_0028_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20_00sec_-15_00C_LIGHT_0235_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20_00sec_-15_00C_LIGHT_0029_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20_00sec_-15_00C_LIGHT_0235_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20_00sec_-15_00C_LIGHT_0028_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461124.7539,14.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260325.2539 14.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:09:22.50 +15:57:39.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20_00sec_-15_00C_LIGHT_0235_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20_00sec_-15_00C_LIGHT_0029_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20_00sec_-15_00C_LIGHT_0235_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20_00sec_-15_00C_LIGHT_0028_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20_00sec_-15_00C_LIGHT_0235_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20_00sec_-15_00C_LIGHT_0029_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20_00sec_-15_00C_LIGHT_0235_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20_00sec_-15_00C_LIGHT_0028_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461124.7539,14.34,0.05,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 20260325.2539 14.34CV 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
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:58:56.20 +14:49:06.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20_00sec_-15_00C_LIGHT_0235_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20_00sec_-15_00C_LIGHT_0029_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20_00sec_-15_00C_LIGHT_0235_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20_00sec_-15_00C_LIGHT_0028_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20_00sec_-15_00C_LIGHT_0235_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20_00sec_-15_00C_LIGHT_0029_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20_00sec_-15_00C_LIGHT_0235_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20_00sec_-15_00C_LIGHT_0028_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461124.7539,14.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260325.2539 14.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:01:13.52 +14:53:52.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20_00sec_-15_00C_LIGHT_0235_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20_00sec_-15_00C_LIGHT_0029_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20_00sec_-15_00C_LIGHT_0235_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20_00sec_-15_00C_LIGHT_0028_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20_00sec_-15_00C_LIGHT_0235_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20_00sec_-15_00C_LIGHT_0029_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20_00sec_-15_00C_LIGHT_0235_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20_00sec_-15_00C_LIGHT_0028_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461082.75729163 11.02.2026 06:10:19.997 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
First image: 2461082.75729163 11.02.2026 06:10:19.997 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
Last image: 2461124.75411175 25.03.2026 06:05:45.255 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.61
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: 3 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): 8713
Objects passed selection criteria: 8682
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 6785.75
Average stars matched: 6455.25 (95.1295 %)
Memory usage VmPeak: 114408 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Mar 25 01:16:05 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: 2461082.75729163 11.02.2026 06:10:19.997 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
First image: 2461082.75729163 11.02.2026 06:10:19.997 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
Last image: 2461124.75411175 25.03.2026 06:05:45.255 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 38
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.27
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): 55712
Objects passed selection criteria: 55550
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 43926
Average stars matched: 41610.5 (94.7286 %)
Memory usage VmPeak: 154532 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Mar 25 01:16:59 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/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits
SExtractor catalog cache: saved Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat to cache
SExtractor catalog cache: saved Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.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/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.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: 2461124.75360302
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'
Plate-solving the images
wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits exists and is non-empty
Saving wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits to local_wcs_cache/
'wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits' -> 'local_wcs_cache/wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits'
wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits exists and is non-empty
Saving wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits to local_wcs_cache/
'wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits' -> 'local_wcs_cache/wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits'
wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits exists and is non-empty
Saving wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits to local_wcs_cache/
'wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits' -> 'local_wcs_cache/wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits'
wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits exists and is non-empty
Saving wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits to local_wcs_cache/
'wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits' -> 'local_wcs_cache/wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:53:20.681 +13:59:51.92
Second-epoch image center 08:53:41.699 +14:01:28.40
Angular distance between the image centers 0.09 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:53:20.681 +13:59:51.92
Second-epoch image center 08:53:42.476 +14:01:25.72
Angular distance between the image centers 0.09 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 08:53:41.699 +14:01:28.40
Second-epoch second image center 08:53:42.476 +14:01:25.72
Angular distance between the image centers 0.00323 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/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits &> /tmp/tmp.8JZWKLjGpf
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits &> /tmp/tmp.SWKFnHJsRD
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits &> /tmp/tmp.Ppnv3AOW4k
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits &> /tmp/tmp.39hhlHBTJ6
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits
Calibrating the magnitude scale
Found non-empty wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.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_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits and wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.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_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits and wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat
Found non-empty wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits and wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat
The reference image (wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits) and catalog (wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat) found
'wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat' -> 'wcsmag.cat'
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
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 5900 out of 9772 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.809505
a=0.000000 b=1.000000 c=22.809505
From vast_summary.log: estimated ref. image limiting mag.: -7.61
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.20
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.20
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
2.0 pix Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
2.4 pix fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits
2.4 pix fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits
Limiting magnitude estimates:
15.2 mag. Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
15.2 mag. Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
14.4 mag. fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits
14.4 mag. fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits
All-image limiting magnitude estimate: 14.4 (SNR ) 11.6 (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.8JZWKLjGpf (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits' -> 'wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
WCS_IMAGE_NAME=wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
WCS-calibrated image found: wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
Checking if the catalog wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat corresponding to the image wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits alredy exist and is non-empty...
Catalog wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat corresponding to the image wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
WCS catalog name: wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=759, passed=9772
Got 9772 stars (including 8997 good ones) from the SExtractor catalog wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat
util/solve_plate_with_UCAC5 got 9772 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.36"
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits -region wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.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.SWKFnHJsRD (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits' -> 'wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
WCS_IMAGE_NAME=wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
WCS-calibrated image found: wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
Checking if the catalog wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits.cat corresponding to the image wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits alredy exist and is non-empty...
Catalog wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits.cat corresponding to the image wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
WCS catalog name: wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=774, passed=9656
Got 9656 stars (including 8873 good ones) from the SExtractor catalog wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits.cat
util/solve_plate_with_UCAC5 got 9656 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
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...
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.38"
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits -region wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.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.Ppnv3AOW4k (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_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.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_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits
WCS-calibrated image found: wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits
Checking if the catalog wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits.cat corresponding to the image wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits.cat corresponding to the image wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits
WCS catalog name: wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=377, passed=6391
Got 6391 stars (including 6008 good ones) from the SExtractor catalog wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits.cat
util/solve_plate_with_UCAC5 got 6391 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
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...
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
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...
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.50"
Estimated accuracy of the plate solution: 0.53"
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_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits -region wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.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.39hhlHBTJ6 (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_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.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_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits
WCS-calibrated image found: wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits
Checking if the catalog wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits.cat corresponding to the image wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits.cat corresponding to the image wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits
WCS catalog name: wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=391, passed=6443
Got 6443 stars (including 6047 good ones) from the SExtractor catalog wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits.cat
util/solve_plate_with_UCAC5 got 6443 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
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...
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.51"
Estimated accuracy of the plate solution: 0.53"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits -region wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.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_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits'
Saving fully-calibrated image wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits'
Saving fully-calibrated image wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits'
Saving fully-calibrated image wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits'
Preparing the HTML report for the field Cnc-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20411_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029
The candidate 20411_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029 did not pass the final checks
**** FOUND 08:36:06.79 +10:20:42.5 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Cnc-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits
SExtractor catalog cache: saved Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat to cache
SExtractor catalog cache: saved Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
Creating symlink local_wcs_cache/wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.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_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits exists and is non-empty
wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits exists and is non-empty
wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits exists and is non-empty
wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:53:20.681 +13:59:51.92
Second-epoch image center 08:53:41.699 +14:01:28.40
Angular distance between the image centers 0.09 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:53:20.681 +13:59:51.92
Second-epoch image center 08:53:42.476 +14:01:25.72
Angular distance between the image centers 0.09 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 08:53:41.699 +14:01:28.40
Second-epoch second image center 08:53:42.476 +14:01:25.72
Angular distance between the image centers 0.00323 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/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits &> /tmp/tmp.LKkekJgODb
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits &> /tmp/tmp.Yb0hHQBKgw
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits &> /tmp/tmp.UMpc9fxptD
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits &> /tmp/tmp.9nQ52HTb3Y
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits
Calibrating the magnitude scale
Found non-empty wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.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_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits and wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.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_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits and wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat
Found non-empty wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits and wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat
The reference image (wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits) and catalog (wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat) found
'wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat' -> 'wcsmag.cat'
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
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 6038 out of 61604 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.669299
a=0.000000 b=1.000000 c=22.669299
From vast_summary.log: estimated ref. image limiting mag.: -7.27
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.40
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.40
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 29 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.8 pix Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
1.8 pix Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
2.2 pix fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits
2.2 pix fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits
Limiting magnitude estimates:
15.4 mag. Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
15.4 mag. Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
14.6 mag. fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits
14.6 mag. fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 14.1 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.LKkekJgODb (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits' -> 'wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
WCS_IMAGE_NAME=wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
WCS-calibrated image found: wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
Checking if the catalog wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat corresponding to the image wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits alredy exist and is non-empty...
Catalog wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat corresponding to the image wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
WCS catalog name: wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=3469, passed=61585
Got 61585 stars (including 58012 good ones) from the SExtractor catalog wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat
util/solve_plate_with_UCAC5 got 61585 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.39"
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits -region wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.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.Yb0hHQBKgw (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits' -> 'wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
WCS_IMAGE_NAME=wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
WCS-calibrated image found: wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
Checking if the catalog wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits.cat corresponding to the image wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits alredy exist and is non-empty...
Catalog wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits.cat corresponding to the image wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
WCS catalog name: wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=23, blended=3459, passed=61573
Got 61573 stars (including 57999 good ones) from the SExtractor catalog wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits.cat
util/solve_plate_with_UCAC5 got 61573 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.39"
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits -region wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.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.UMpc9fxptD (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_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.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_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits
WCS-calibrated image found: wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits
Checking if the catalog wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits.cat corresponding to the image wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits.cat corresponding to the image wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits
WCS catalog name: wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=1522, passed=36562
Got 36562 stars (including 34996 good ones) from the SExtractor catalog wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits.cat
util/solve_plate_with_UCAC5 got 36562 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
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...
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.47"
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...
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.47"
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_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits -region wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.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.9nQ52HTb3Y (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_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.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_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits
WCS-calibrated image found: wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits
Checking if the catalog wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits.cat corresponding to the image wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits.cat corresponding to the image wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits
WCS catalog name: wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=1609, passed=37042
Got 37042 stars (including 35389 good ones) from the SExtractor catalog wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits.cat
util/solve_plate_with_UCAC5 got 37042 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010413 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
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...
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
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...
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.48"
Estimated accuracy of the plate solution: 0.50"
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_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits -region wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.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_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.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_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
Saving fully-calibrated image wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.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_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
Saving fully-calibrated image wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.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_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-01_20.00sec_-15.00C_LIGHT_0028.fits
Saving fully-calibrated image wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.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_2026-03-25_CI_Cnc-05-Q2b1x1_011355_TTUQ2b1x1_15585_c6O1SkHq/wcs_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029.fits
Preparing the HTML report for the field Cnc-05-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out75717.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75721.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out77119.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out77380.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out77652.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78050.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78076.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78278.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78431.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78535.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78699.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78928.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79213.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79215.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out80166.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out80203.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out80376.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out77655.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79878.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out80124.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out80127.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: 2s
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Considering the candidate 75717_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029
The candidate 75717_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029 did not pass the final checks
**** FOUND 08:40:36.33 +15:20:51.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)GAIADR2_OUTPUT=# 0.330 657679550239624960 130.15135300840 +15.34783924406 13.6438 13.0116 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.330#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 75721_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029
The candidate 75721_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029 did not pass the final checks
**** FOUND 09:07:53.19 +13:56:33.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)GAIADR2_OUTPUT=# 1.254 606911490612013696 136.97196028995 +13.94284638944 14.3873 13.8861 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.254#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 77119_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029
The candidate 77119_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029 did not pass the final checks
**** FOUND 08:51:25.93 +11:49:09.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)
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Considering the candidate 77380_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029
The candidate 77380_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029 did not pass the final checks
**** FOUND 09:10:21.03 +13:22:52.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 1.491 606080019303389824 137.58724141657 +13.38131854031 13.1700 12.7079 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.491#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 77652_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029
The candidate 77652_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029 did not pass the final checks
**** FOUND 08:43:45.63 +11:14:56.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 1.323 601822779000393472 130.93985239295 +11.24888661242 13.0921 12.6610 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.323#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 77655_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029
Preparing report for the candidate 77655_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029
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Considering the candidate 77715_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029
The candidate 77715_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 77733_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029
The candidate 77733_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 78050_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029
The candidate 78050_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029 did not pass the final checks
**** FOUND 08:49:32.79 +12:08:57.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 0.842 604986172737115904 132.38650283364 +12.14936791624 13.0569 12.5497 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.842#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 78076_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029
The candidate 78076_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029 did not pass the final checks
**** FOUND 09:11:17.03 +15:03:28.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 1.072 607457844811803136 137.82067908989 +15.05798766165 13.5690 13.1699 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.072#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 78278_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029
The candidate 78278_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029 did not pass the final checks
**** FOUND 08:43:08.96 +14:05:36.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 0.613 609224897437415680 130.78717735122 +14.09350545346 13.5505 13.2268 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.613#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 78431_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029
The candidate 78431_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029 did not pass the final checks
**** FOUND 08:51:16.38 +11:44:33.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)GAIADR2_OUTPUT=# 1.832 604911199788235648 132.81779812771 +11.74247063470 13.3138 12.8480 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.832#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 78535_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029
The candidate 78535_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029 did not pass the final checks
**** FOUND 08:36:44.39 +13:59:11.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 3.686 603429406007141376 129.18570754641 +13.98566803482 13.7018 13.0880 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.686#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 78699_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029
The candidate 78699_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029 did not pass the final checks
**** FOUND 09:05:14.14 +14:15:45.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 0.892 606996462244963584 136.30884858484 +14.26276662089 13.7297 13.2769 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.892#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 78780_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029
The candidate 78780_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 78879_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029
The candidate 78879_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029 did not pass the final checks
**** FOUND 08:49:56.28 +14:48:29.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78928_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029
The candidate 78928_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029 did not pass the final checks
**** FOUND 08:48:10.86 +15:04:59.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 1.416 609757335943320320 132.04561225773 +15.08287572126 14.0144 13.5382 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.416#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 78933_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029
The candidate 78933_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 79213_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029
The candidate 79213_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029 did not pass the final checks
**** FOUND 08:45:55.23 +11:26:04.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 0.950 601934306415252096 131.47988913147 +11.43476590196 14.0606 13.6333 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.950#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79215_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029
The candidate 79215_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029 did not pass the final checks
**** FOUND 08:43:52.58 +10:16:01.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 2.117 598335261260205056 130.96880707019 +10.26647849969 13.8313 13.2885 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.117#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79453_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029
The candidate 79453_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 79878_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029
Preparing report for the candidate 79878_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029
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Considering the candidate 80121_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029
The candidate 80121_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 80124_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029
Preparing report for the candidate 80124_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029
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Considering the candidate 80127_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029
Preparing report for the candidate 80127_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029
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Considering the candidate 80166_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029
The candidate 80166_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029 did not pass the final checks
**** FOUND 08:46:05.47 +11:58:32.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)GAIADR2_OUTPUT=# 1.527 601968292492213632 131.52321439355 +11.97581649634 14.5402 14.0142 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.527#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 80203_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029
The candidate 80203_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029 did not pass the final checks
**** FOUND 09:14:07.11 +15:23:19.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.47, MAG_FAINT_SEARCH_LIMIT=15.45)GAIADR2_OUTPUT=# 1.951 607572430244321536 138.52945977499 +15.38924029646 14.3592 13.5772 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.951#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 80303_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029
The candidate 80303_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 80376_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029
The candidate 80376_fd_Cnc-05-Q2b1x1_2026-03-25_01-05-45_20.00sec_-15.00C_LIGHT_0029 did not pass the final checks