This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3
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
NSVS J0514205+695157,2461129.6576,12.76,0.05,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
NSVS J0514205+695157 20260330.1576 12.76CV 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/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:14:19.98 +69:51:57.0 ;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_Cam-06-Q2b1x1_2026-01-08_22-41-51_20_00sec_-14_90C_LIGHT_0169_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20_00sec_-10_00C_LIGHT_0123_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20_00sec_-14_90C_LIGHT_0169_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20_00sec_-10_00C_LIGHT_0122_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20_00sec_-14_90C_LIGHT_0169_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20_00sec_-10_00C_LIGHT_0123_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20_00sec_-14_90C_LIGHT_0169_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20_00sec_-10_00C_LIGHT_0122_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
NSVS J0418017+711356,2461129.6576,12.57,0.05,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
NSVS J0418017+711356 20260330.1576 12.57CV 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/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:18:00.94 +71:13:51.8 ;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_Cam-06-Q2b1x1_2026-01-08_22-41-51_20_00sec_-14_90C_LIGHT_0169_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20_00sec_-10_00C_LIGHT_0123_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20_00sec_-14_90C_LIGHT_0169_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20_00sec_-10_00C_LIGHT_0122_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20_00sec_-14_90C_LIGHT_0169_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20_00sec_-10_00C_LIGHT_0123_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20_00sec_-14_90C_LIGHT_0169_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20_00sec_-10_00C_LIGHT_0122_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
NSVS J0437484+693139,2461129.6576,12.17,0.05,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
NSVS J0437484+693139 20260330.1576 12.17CV 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/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:37:49.01 +69:31:38.3 ;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_Cam-06-Q2b1x1_2026-01-08_22-41-51_20_00sec_-14_90C_LIGHT_0169_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20_00sec_-10_00C_LIGHT_0123_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20_00sec_-14_90C_LIGHT_0169_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20_00sec_-10_00C_LIGHT_0122_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20_00sec_-14_90C_LIGHT_0169_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20_00sec_-10_00C_LIGHT_0123_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20_00sec_-14_90C_LIGHT_0169_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20_00sec_-10_00C_LIGHT_0122_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: 2461049.69585608 09.01.2026 04:41:51.965 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
First image: 2461049.69585608 09.01.2026 04:41:51.965 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
Last image: 2461129.65791045 30.03.2026 03:47:13.463 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.51
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: 5 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): 14293
Objects passed selection criteria: 14233
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 10083.8
Average stars matched: 9746 (96.6506 %)
Memory usage VmPeak: 120264 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 Sun Mar 29 22:51:18 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: 2461049.69585608 09.01.2026 04:41:51.965 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
First image: 2461049.69585608 09.01.2026 04:41:51.965 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
Last image: 2461129.65791045 30.03.2026 03:47:13.463 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 64
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.18
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): 99307
Objects passed selection criteria: 99036
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 72366
Average stars matched: 69538 (96.0921 %)
Memory usage VmPeak: 2324220 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 Sun Mar 29 22:58:09 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/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits
SExtractor catalog cache: saved Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits.cat to cache
SExtractor catalog cache: saved Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.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/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.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: 2461129.65731105
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_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits exists and is non-empty
Saving wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits to local_wcs_cache/
'wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits' -> 'local_wcs_cache/wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits'
wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits exists and is non-empty
Saving wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits to local_wcs_cache/
'wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits' -> 'local_wcs_cache/wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits'
wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits exists and is non-empty
Saving wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits to local_wcs_cache/
'wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits' -> 'local_wcs_cache/wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits'
wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits exists and is non-empty
Saving wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits to local_wcs_cache/
'wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits' -> 'local_wcs_cache/wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.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 04:47:16.792 +69:58:46.61
Second-epoch image center 04:48:00.122 +70:00:24.74
Angular distance between the image centers 0.07 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 04:47:16.792 +69:58:46.61
Second-epoch image center 04:48:02.519 +70:00:14.16
Angular distance between the image centers 0.07 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 04:48:00.122 +70:00:24.74
Second-epoch second image center 04:48:02.519 +70:00:14.16
Angular distance between the image centers 0.00451 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/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits &> /tmp/tmp.5qk0riWWzF
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits &> /tmp/tmp.FJ2iocSp29
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits &> /tmp/tmp.26931Rg7pj
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits &> /tmp/tmp.kWPE0NLYpm
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits
Calibrating the magnitude scale
Found non-empty wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.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_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits and wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.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_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits and wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits.cat
Found non-empty wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits and wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits.cat
The reference image (wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits) and catalog (wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits.cat) found
'wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.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 8346 out of 17535 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.930229
a=0.000000 b=1.000000 c=22.930229
From vast_summary.log: estimated ref. image limiting mag.: -7.51
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.42
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.42
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
2.0 pix Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
2.5 pix fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits
2.5 pix fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits
Limiting magnitude estimates:
15.4 mag. Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
15.4 mag. Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
14.0 mag. fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits
14.0 mag. fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 11.2 (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.5qk0riWWzF (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/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.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_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits' -> 'wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
WCS_IMAGE_NAME=wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
WCS-calibrated image found: wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
Checking if the catalog wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits alredy exist and is non-empty...
Catalog wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
WCS catalog name: wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1440, passed=17535
Got 17535 stars (including 16074 good ones) from the SExtractor catalog wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits.cat
util/solve_plate_with_UCAC5 got 17535 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 970 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: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
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 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.32"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits -region wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.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.FJ2iocSp29 (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/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.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_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits' -> 'wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
WCS_IMAGE_NAME=wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
WCS-calibrated image found: wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
Checking if the catalog wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits alredy exist and is non-empty...
Catalog wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
WCS catalog name: wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1424, passed=17523
Got 17523 stars (including 16079 good ones) from the SExtractor catalog wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits.cat
util/solve_plate_with_UCAC5 got 17523 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 971 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: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
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 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.32"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits -region wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.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.26931Rg7pj (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_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.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_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits
WCS_IMAGE_NAME=wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits
WCS-calibrated image found: wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits
Checking if the catalog wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits.cat corresponding to the image wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits.cat corresponding to the image wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits
WCS catalog name: wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=373, passed=5933
Got 5933 stars (including 5552 good ones) from the SExtractor catalog wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits.cat
util/solve_plate_with_UCAC5 got 5933 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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 966 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: 0.52"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.53"
Estimated accuracy of the plate solution: 0.56"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits -region wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.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.kWPE0NLYpm (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_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.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_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits
WCS_IMAGE_NAME=wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits
WCS-calibrated image found: wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits
Checking if the catalog wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits.cat corresponding to the image wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits.cat corresponding to the image wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits
WCS catalog name: wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=375, passed=5894
Got 5894 stars (including 5515 good ones) from the SExtractor catalog wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits.cat
util/solve_plate_with_UCAC5 got 5894 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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 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: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
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: 0.53"
Estimated accuracy of the plate solution: 0.55"
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_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits -region wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.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_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits'
Saving fully-calibrated image wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits'
Saving fully-calibrated image wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits'
Saving fully-calibrated image wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits'
Preparing the HTML report for the field Cam-06-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Cam-06-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/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits
SExtractor catalog cache: saved Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits.cat to cache
SExtractor catalog cache: saved Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
Creating symlink local_wcs_cache/wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
Creating symlink local_wcs_cache/wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits
Creating symlink local_wcs_cache/wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.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_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits exists and is non-empty
wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits exists and is non-empty
wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits exists and is non-empty
wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.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 04:47:16.792 +69:58:46.61
Second-epoch image center 04:48:00.122 +70:00:24.74
Angular distance between the image centers 0.07 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 04:47:16.792 +69:58:46.61
Second-epoch image center 04:48:02.519 +70:00:14.16
Angular distance between the image centers 0.07 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 04:48:00.122 +70:00:24.74
Second-epoch second image center 04:48:02.519 +70:00:14.16
Angular distance between the image centers 0.00451 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/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits &> /tmp/tmp.yoCfM0G3mV
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits &> /tmp/tmp.3SnbwMSF8c
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits &> /tmp/tmp.yqL8lDP5fz
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits &> /tmp/tmp.DQ1Co1jvJY
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits
Calibrating the magnitude scale
Found non-empty wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.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_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits and wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.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_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits and wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits.cat
Found non-empty wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits and wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits.cat
The reference image (wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits) and catalog (wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits.cat) found
'wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.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 8413 out of 121322 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.798908
a=0.000000 b=1.000000 c=22.798908
From vast_summary.log: estimated ref. image limiting mag.: -7.18
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.62
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.62
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 52 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
1.9 pix Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
2.3 pix fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits
2.3 pix fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits
Limiting magnitude estimates:
15.6 mag. Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
15.6 mag. Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
14.1 mag. fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits
14.1 mag. fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 13.6 (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.yoCfM0G3mV (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/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.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_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits' -> 'wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
WCS_IMAGE_NAME=wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
WCS-calibrated image found: wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
Checking if the catalog wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits alredy exist and is non-empty...
Catalog wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
WCS catalog name: wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=10875, passed=121302
Got 121302 stars (including 110227 good ones) from the SExtractor catalog wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits.cat
util/solve_plate_with_UCAC5 got 121302 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 971 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: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.35"
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits -region wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.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.3SnbwMSF8c (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/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.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_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits' -> 'wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
WCS_IMAGE_NAME=wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
WCS-calibrated image found: wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
Checking if the catalog wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits alredy exist and is non-empty...
Catalog wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
WCS catalog name: wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=28, blended=10830, passed=121526
Got 121526 stars (including 110505 good ones) from the SExtractor catalog wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits.cat
util/solve_plate_with_UCAC5 got 121526 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (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 971 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: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.35"
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits -region wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.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.yqL8lDP5fz (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_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.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_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits
WCS_IMAGE_NAME=wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits
WCS-calibrated image found: wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits
Checking if the catalog wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits.cat corresponding to the image wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits.cat corresponding to the image wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits
WCS catalog name: wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=2015, passed=40432
Got 40432 stars (including 38374 good ones) from the SExtractor catalog wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits.cat
util/solve_plate_with_UCAC5 got 40432 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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 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: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.53"
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: 0.53"
Estimated accuracy of the plate solution: 0.57"
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_fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits -region wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.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.DQ1Co1jvJY (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_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.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_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits
WCS_IMAGE_NAME=wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits
WCS-calibrated image found: wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits
Checking if the catalog wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits.cat corresponding to the image wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits.cat corresponding to the image wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits
WCS catalog name: wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=4, blended=2166, passed=41468
Got 41468 stars (including 39270 good ones) from the SExtractor catalog wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits.cat
util/solve_plate_with_UCAC5 got 41468 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (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 0.010414 (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: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
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: 0.52"
Estimated accuracy of the plate solution: 0.55"
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_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits -region wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.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_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.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_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/wcs_Cam-06-Q2b1x1_2026-01-08_22-41-51_20.00sec_-14.90C_LIGHT_0169.fits
Saving fully-calibrated image wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.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_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/wcs_Cam-06-Q2b1x1_2026-01-08_22-42-29_20.00sec_-15.00C_LIGHT_0170.fits
Saving fully-calibrated image wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.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_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-46-21_20.00sec_-10.00C_LIGHT_0122.fits
Saving fully-calibrated image wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.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_2026-03-29_CI_Cam-06-Q2b1x1_224904_TTUQ2b1x1_580_sAvwUTz3/wcs_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123.fits
Preparing the HTML report for the field Cam-06-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out140698.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out140706.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out140709.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out140712.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out141835.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out141914.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out142066.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out142121.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out142186.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out142230.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out46725.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55699.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out66789.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 140698_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
The candidate 140698_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123 did not pass the final checks
**** FOUND 03:54:51.32 +70:05:01.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)
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Considering the candidate 140704_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
The candidate 140704_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123 did not pass the final checks
**** FOUND 04:34:33.92 +65:47:40.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 140706_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
The candidate 140706_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123 did not pass the final checks
**** FOUND 04:34:26.69 +71:29:04.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 1.059 500550542539857792 068.61213416316 +71.48446342110 13.2803 12.7020 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.059#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 140709_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
The candidate 140709_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123 did not pass the final checks
**** FOUND 05:10:17.05 +68:51:07.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 0.849 485549939761973888 077.57068644050 +68.85182967008 13.0308 12.5583 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.849#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 140711_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
The candidate 140711_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123 did not pass the final checks
**** FOUND 05:02:20.61 +72:25:36.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 140712_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
The candidate 140712_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123 did not pass the final checks
**** FOUND 04:05:41.13 +69:16:46.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)GAIADR2_OUTPUT=# 2.387 493935979369184384 061.42038916027 +69.27899180711 12.1103 11.3655 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.387#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 141269_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
The candidate 141269_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
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Considering the candidate 141409_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
The candidate 141409_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123 did not pass the final checks
**** FOUND 04:59:57.72 +70:27:21.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 141482_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
The candidate 141482_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123 did not pass the final checks
**** FOUND 04:13:20.28 +72:06:35.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 141498_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
The candidate 141498_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123 did not pass the final checks
**** FOUND 05:03:07.96 +66:49:08.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 141510_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
The candidate 141510_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123 did not pass the final checks
**** FOUND 03:52:25.27 +67:32:43.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 141533_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
The candidate 141533_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123 did not pass the final checks
**** FOUND 04:51:34.12 +68:12:02.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 141561_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
The candidate 141561_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123 did not pass the final checks
**** FOUND 04:50:06.13 +66:30:50.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 141570_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
The candidate 141570_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123 did not pass the final checks
**** FOUND 04:53:50.63 +66:22:13.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 141634_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
The candidate 141634_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123 did not pass the final checks
**** FOUND 04:51:32.92 +68:11:47.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 141661_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
The candidate 141661_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123 did not pass the final checks
**** FOUND 06:07:06.54 +72:35:30.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 141744_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
The candidate 141744_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123 did not pass the final checks
**** FOUND 05:44:56.76 +67:59:48.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 141746_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
The candidate 141746_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123 did not pass the final checks
**** FOUND 04:54:09.89 +66:18:59.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 141785_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
The candidate 141785_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123 did not pass the final checks
**** FOUND 05:13:53.99 +67:29:16.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 141803_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
The candidate 141803_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123 did not pass the final checks
**** FOUND 05:42:25.41 +71:17:33.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 141835_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
The candidate 141835_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123 did not pass the final checks
**** FOUND 04:48:32.10 +67:45:37.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 1.257 483568207492751488 072.13463818979 +67.76053838622 12.8671 12.0644 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.257#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 141872_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
The candidate 141872_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123 did not pass the final checks
**** FOUND 06:12:19.38 +72:27:30.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 141877_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
The candidate 141877_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123 did not pass the final checks
**** FOUND 04:09:45.84 +68:22:46.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 141907_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
The candidate 141907_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123 did not pass the final checks
**** FOUND 04:13:40.89 +72:09:24.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 141914_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
The candidate 141914_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123 did not pass the final checks
**** FOUND 05:42:45.59 +71:17:38.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 3.577 486227513802366592 085.69239557328 +71.29450224591 13.1826 12.5195 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.577#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 141953_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
The candidate 141953_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123 did not pass the final checks
**** FOUND 06:05:56.28 +69:29:32.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 142003_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
The candidate 142003_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123 did not pass the final checks
**** FOUND 04:02:58.15 +72:49:33.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 142026_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
The candidate 142026_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123 did not pass the final checks
**** FOUND 04:17:16.42 +66:57:57.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 142066_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
The candidate 142066_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123 did not pass the final checks
**** FOUND 04:30:54.02 +70:19:53.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)GAIADR2_OUTPUT=# 0.843 497042928648960768 067.72438826472 +70.33148097797 13.0976 12.4382 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.843#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 142102_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
The candidate 142102_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123 did not pass the final checks
**** FOUND 05:21:53.99 +67:02:55.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 142121_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
The candidate 142121_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123 did not pass the final checks
**** FOUND 05:39:26.22 +69:52:42.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)GAIADR2_OUTPUT=# 1.186 485841722660852224 084.85947568822 +69.87882015712 14.0568 12.9980 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.186#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 142166_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
The candidate 142166_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123 did not pass the final checks
**** FOUND 05:19:26.59 +67:59:46.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 142169_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
The candidate 142169_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123 did not pass the final checks
**** FOUND 05:02:40.44 +66:48:09.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 142178_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
The candidate 142178_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123 did not pass the final checks
**** FOUND 05:37:29.08 +66:41:32.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 142186_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
The candidate 142186_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123 did not pass the final checks
**** FOUND 04:59:24.32 +66:23:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 0.244 482784221342554496 074.85127181760 +66.39638141604 13.7055 13.1447 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.244#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 142193_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
The candidate 142193_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123 did not pass the final checks
**** FOUND 05:14:25.70 +69:50:41.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 142203_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
The candidate 142203_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123 did not pass the final checks
Rejecting candidate due to large distance (17.2") between the two second-epoch detections
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Considering the candidate 142227_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
The candidate 142227_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123 did not pass the final checks
**** FOUND 05:42:48.32 +71:16:35.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 142230_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
The candidate 142230_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123 did not pass the final checks
**** FOUND 05:14:24.29 +66:26:37.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 3.237 482635924712800384 078.60292475051 +66.44444242367 13.7615 13.1874 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.237#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 142244_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
The candidate 142244_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123 did not pass the final checks
**** FOUND 04:13:32.41 +72:06:03.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 142258_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
The candidate 142258_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123 did not pass the final checks
**** FOUND 05:20:28.68 +71:45:08.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 142260_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
The candidate 142260_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
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Considering the candidate 142262_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
The candidate 142262_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123 did not pass the final checks
**** FOUND 05:22:35.57 +67:04:22.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 142342_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
The candidate 142342_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123 did not pass the final checks
Rejecting candidate due to large distance (18.6") between the two second-epoch detections
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Considering the candidate 142350_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
The candidate 142350_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123 did not pass the final checks
**** FOUND 05:22:04.18 +70:19:57.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 142404_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
The candidate 142404_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
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Considering the candidate 142415_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
The candidate 142415_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123 did not pass the final checks
Rejecting candidate due to large distance (16.8") between the two second-epoch detections
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Considering the candidate 142425_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
The candidate 142425_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123 did not pass the final checks
**** FOUND 05:08:13.26 +69:55:47.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 55699_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
Preparing report for the candidate 55699_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
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Considering the candidate 46725_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
Preparing report for the candidate 46725_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
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Considering the candidate 66789_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
Preparing report for the candidate 66789_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
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Considering the candidate 85227_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123
The candidate 85227_fd_Cam-06-Q2b1x1_2026-03-29_22-47-13_20.00sec_-10.00C_LIGHT_0123 did not pass the final checks