This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461125.6499,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260326.1499 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:36:44.66 +15:55:22.0 ;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_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20_00sec_-15_00C_LIGHT_0235_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20_00sec_-10_00C_LIGHT_0345_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20_00sec_-15_00C_LIGHT_0235_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20_00sec_-10_00C_LIGHT_0344_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20_00sec_-15_00C_LIGHT_0235_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20_00sec_-10_00C_LIGHT_0345_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20_00sec_-15_00C_LIGHT_0235_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20_00sec_-10_00C_LIGHT_0344_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461125.6499,14.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260326.1499 14.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:58:41.13 +14:47:02.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20_00sec_-15_00C_LIGHT_0235_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20_00sec_-10_00C_LIGHT_0345_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20_00sec_-15_00C_LIGHT_0235_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20_00sec_-10_00C_LIGHT_0344_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20_00sec_-15_00C_LIGHT_0235_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20_00sec_-10_00C_LIGHT_0345_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20_00sec_-15_00C_LIGHT_0235_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20_00sec_-10_00C_LIGHT_0344_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461125.6499,14.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260326.1499 14.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:01:06.35 +14:55:35.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20_00sec_-15_00C_LIGHT_0235_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20_00sec_-10_00C_LIGHT_0345_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20_00sec_-15_00C_LIGHT_0235_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20_00sec_-10_00C_LIGHT_0344_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20_00sec_-15_00C_LIGHT_0235_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20_00sec_-10_00C_LIGHT_0345_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20_00sec_-15_00C_LIGHT_0235_fits__*pix.png resample_wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20_00sec_-10_00C_LIGHT_0344_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461082.75729163 11.02.2026 06:10:19.997 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
First image: 2461082.75729163 11.02.2026 06:10:19.997 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
Last image: 2461125.65019667 26.03.2026 03:36:06.992 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.61
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 9183
Objects passed selection criteria: 9161
Measurements per detected object (mean, median, min, max): 3.3 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.3 4.0 2 4
Average stars detected per image: 7697
Average stars matched: 7290 (94.7122 %)
Memory usage VmPeak: 114404 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Mar 25 22:45:23 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461082.75729163 11.02.2026 06:10:19.997 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
First image: 2461082.75729163 11.02.2026 06:10:19.997 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
Last image: 2461125.65019667 26.03.2026 03:36:06.992 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 81
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.27
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 15 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): 56514
Objects passed selection criteria: 56332
Measurements per detected object (mean, median, min, max): 3.2 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.2 4.0 2 4
Average stars detected per image: 46633
Average stars matched: 44200.2 (94.7832 %)
Memory usage VmPeak: 154532 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Mar 25 22:46:13 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits
SExtractor catalog cache: saved Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat to cache
SExtractor catalog cache: saved Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.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: 2461125.64966857
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits exists and is non-empty
Saving wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits to local_wcs_cache/
'wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits' -> 'local_wcs_cache/wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits'
wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits exists and is non-empty
Saving wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits to local_wcs_cache/
'wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits' -> 'local_wcs_cache/wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits'
wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits exists and is non-empty
Saving wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits to local_wcs_cache/
'wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits' -> 'local_wcs_cache/wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits'
wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits exists and is non-empty
Saving wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits to local_wcs_cache/
'wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits' -> 'local_wcs_cache/wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:53:20.681 +13:59:51.92
Second-epoch image center 08:53:36.546 +14:02:28.72
Angular distance between the image centers 0.08 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:53:20.681 +13:59:51.92
Second-epoch image center 08:53:35.953 +14:02:29.24
Angular distance between the image centers 0.08 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 08:53:36.546 +14:02:28.72
Second-epoch second image center 08:53:35.953 +14:02:29.24
Angular distance between the image centers 0.00240 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits &> /tmp/tmp.sE3FCg4d0i
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits &> /tmp/tmp.qRPy85UMqp
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits &> /tmp/tmp.2CjZ1DqOZW
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits &> /tmp/tmp.FkgQlUDiuf
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits
Calibrating the magnitude scale
Found non-empty wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits and wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits and wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat
Found non-empty wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits and wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat
The reference image (wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits) and catalog (wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat) found
'wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat' -> 'wcsmag.cat'
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 5900 out of 9772 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.809505
a=0.000000 b=1.000000 c=22.809505
From vast_summary.log: estimated ref. image limiting mag.: -7.61
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.20
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.20
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
2.0 pix Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
2.7 pix fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits
2.6 pix fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits
Limiting magnitude estimates:
15.2 mag. Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
15.2 mag. Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
14.8 mag. fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits
14.9 mag. fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 12.0 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.sE3FCg4d0i (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits' -> 'wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
WCS_IMAGE_NAME=wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
WCS-calibrated image found: wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
Checking if the catalog wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat corresponding to the image wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits alredy exist and is non-empty...
Catalog wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat corresponding to the image wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
WCS catalog name: wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=759, passed=9772
Got 9772 stars (including 8997 good ones) from the SExtractor catalog wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat
util/solve_plate_with_UCAC5 got 9772 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.36"
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits -region wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.qRPy85UMqp (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits' -> 'wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
WCS_IMAGE_NAME=wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
WCS-calibrated image found: wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
Checking if the catalog wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits.cat corresponding to the image wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits alredy exist and is non-empty...
Catalog wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits.cat corresponding to the image wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
WCS catalog name: wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=774, passed=9656
Got 9656 stars (including 8873 good ones) from the SExtractor catalog wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits.cat
util/solve_plate_with_UCAC5 got 9656 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.38"
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits -region wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.2CjZ1DqOZW (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits
WCS-calibrated image found: wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits
Checking if the catalog wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits.cat corresponding to the image wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits.cat corresponding to the image wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits
WCS catalog name: wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=496, passed=8673
Got 8673 stars (including 8162 good ones) from the SExtractor catalog wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits.cat
util/solve_plate_with_UCAC5 got 8673 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 931.8'
Seting catalog search parameters based on the expected field of view 931.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012942 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010353 (37.3 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 760 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 1.81"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 1.89"
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 774 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 1.82"
Estimated accuracy of the plate solution: 1.16"
Excluding outliers - 771 stars left (next iteration limit 830)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits -region wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.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.FkgQlUDiuf (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits
WCS-calibrated image found: wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits
Checking if the catalog wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits.cat corresponding to the image wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits.cat corresponding to the image wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits
WCS catalog name: wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=519, passed=8602
Got 8602 stars (including 8071 good ones) from the SExtractor catalog wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits.cat
util/solve_plate_with_UCAC5 got 8602 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.56"
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 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.56"
Estimated accuracy of the plate solution: 0.60"
Excluding outliers - 955 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits -region wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits'
Saving fully-calibrated image wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits'
Saving fully-calibrated image wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits'
Saving fully-calibrated image wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits'
Preparing the HTML report for the field Cnc-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out21334.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21364.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21369.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 1s
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: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21334_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 21334_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
**** FOUND 08:49:21.49 +12:04:22.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.15, MAG_FAINT_SEARCH_LIMIT=13.13)GAIADR2_OUTPUT=# 0.707 604984665204470016 132.33945924926 +12.07304023844 12.2229 11.6396 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.707#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21364_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 21364_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
**** FOUND 08:46:37.00 +13:46:26.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 0.110 608496642782554880 131.65414402935 +13.77408979010 12.0842 11.6510 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.110#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21369_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 21369_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
**** FOUND 08:50:02.78 +14:39:11.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 0.964 608932526127319296 132.51162415491 +14.65279072411 12.1206 11.7907 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.964#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Cnc-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits
SExtractor catalog cache: saved Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat to cache
SExtractor catalog cache: saved Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
Creating symlink local_wcs_cache/wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits exists and is non-empty
wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits exists and is non-empty
wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits exists and is non-empty
wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:53:20.681 +13:59:51.92
Second-epoch image center 08:53:36.546 +14:02:28.72
Angular distance between the image centers 0.08 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 08:53:20.681 +13:59:51.92
Second-epoch image center 08:53:35.953 +14:02:29.24
Angular distance between the image centers 0.08 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 08:53:36.546 +14:02:28.72
Second-epoch second image center 08:53:35.953 +14:02:29.24
Angular distance between the image centers 0.00240 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits &> /tmp/tmp.b5gr33BDKY
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits &> /tmp/tmp.ilUdxlWUKx
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits &> /tmp/tmp.vqvdKYQlvp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits &> /tmp/tmp.rQmyUK1cNw
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits
Calibrating the magnitude scale
Found non-empty wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits and wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits and wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat
Found non-empty wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits and wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat
The reference image (wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits) and catalog (wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat) found
'wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat' -> 'wcsmag.cat'
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 6038 out of 61604 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.669299
a=0.000000 b=1.000000 c=22.669299
From vast_summary.log: estimated ref. image limiting mag.: -7.27
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.40
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.40
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 57 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.8 pix Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
1.8 pix Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
2.5 pix fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits
2.4 pix fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits
Limiting magnitude estimates:
15.4 mag. Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
15.4 mag. Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
14.9 mag. fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits
15.0 mag. fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits
All-image limiting magnitude estimate: 14.9 (SNR ) 14.4 (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.b5gr33BDKY (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits' -> 'wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
WCS_IMAGE_NAME=wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
WCS-calibrated image found: wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
Checking if the catalog wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat corresponding to the image wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits alredy exist and is non-empty...
Catalog wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat corresponding to the image wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
WCS catalog name: wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=3469, passed=61585
Got 61585 stars (including 58012 good ones) from the SExtractor catalog wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat
util/solve_plate_with_UCAC5 got 61585 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.39"
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits -region wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.ilUdxlWUKx (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits' -> 'wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
WCS_IMAGE_NAME=wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
WCS-calibrated image found: wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
Checking if the catalog wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits.cat corresponding to the image wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits alredy exist and is non-empty...
Catalog wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits.cat corresponding to the image wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
WCS catalog name: wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=23, blended=3459, passed=61573
Got 61573 stars (including 57999 good ones) from the SExtractor catalog wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits.cat
util/solve_plate_with_UCAC5 got 61573 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.39"
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 961 stars left (next iteration limit 1057)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits -region wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.vqvdKYQlvp (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits
WCS-calibrated image found: wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits
Checking if the catalog wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits.cat corresponding to the image wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits.cat corresponding to the image wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits
WCS catalog name: wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=2292, passed=42966
Got 42966 stars (including 40626 good ones) from the SExtractor catalog wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits.cat
util/solve_plate_with_UCAC5 got 42966 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 931.8'
Seting catalog search parameters based on the expected field of view 931.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012942 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010353 (37.3 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 750 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 1.77"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 1.86"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 775 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 1.84"
Estimated accuracy of the plate solution: 1.07"
Excluding outliers - 770 stars left (next iteration limit 819)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits -region wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.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.rQmyUK1cNw (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits
WCS-calibrated image found: wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits
Checking if the catalog wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits.cat corresponding to the image wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits.cat corresponding to the image wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits
WCS catalog name: wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=2436, passed=44299
Got 44299 stars (including 41814 good ones) from the SExtractor catalog wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits.cat
util/solve_plate_with_UCAC5 got 44299 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 956 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: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.54"
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 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.54"
Estimated accuracy of the plate solution: 0.57"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits -region wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/wcs_Cnc-05-Q2b1x1_2026-02-11_00-10-19_20.00sec_-15.00C_LIGHT_0235.fits
Saving fully-calibrated image wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/wcs_Cnc-05-Q2b1x1_2026-02-11_00-11-00_20.00sec_-14.90C_LIGHT_0236.fits
Saving fully-calibrated image wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-35-21_20.00sec_-10.00C_LIGHT_0344.fits
Saving fully-calibrated image wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Cnc-05-Q2b1x1_224307_TTUQ2b1x1_8601_hMS9Ro5j/wcs_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345.fits
Preparing the HTML report for the field Cnc-05-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out75720.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75721.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75723.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out78522.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79153.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out79722.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out80447.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out80584.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out77500.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out80072.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out80291.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
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 75720_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 75720_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
**** FOUND 08:54:08.81 +10:20:15.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.61, MAG_FAINT_SEARCH_LIMIT=15.59)GAIADR2_OUTPUT=# 3.122 597822686979033984 133.53625168010 +10.33843619637 15.0379 14.4836 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.122#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 75721_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 75721_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
**** FOUND 08:51:12.17 +11:54:39.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.73, MAG_FAINT_SEARCH_LIMIT=15.71)GAIADR2_OUTPUT=# 1.422 604922474077954944 132.80048868823 +11.91122023371 15.0684 14.4982 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.422#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 75723_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 75723_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
**** FOUND 08:42:37.21 +14:20:03.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.41, MAG_FAINT_SEARCH_LIMIT=15.39)GAIADR2_OUTPUT=# 0.649 609249705168460928 130.65519840799 +14.33440290563 14.2422 13.7869 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.649#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 75729_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 75729_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (27.6") between the two second-epoch detections
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Considering the candidate 76334_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 76334_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (63.2") between the two second-epoch detections
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Considering the candidate 76562_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 76562_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 77015_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 77015_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 77283_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 77283_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (57.3") between the two second-epoch detections
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Considering the candidate 77500_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
Preparing report for the candidate 77500_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
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Considering the candidate 77563_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 77563_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
**** FOUND 08:49:32.81 +12:08:57.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 77822_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 77822_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (162.9") between the two second-epoch detections
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Considering the candidate 78164_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 78164_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
**** FOUND 08:43:08.97 +14:05:37.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78479_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 78479_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 78522_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 78522_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
**** FOUND 08:29:22.88 +11:17:03.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 1.844 600944200490992128 127.34554133825 +11.28378011326 13.6924 13.2548 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.844#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 78528_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 78528_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
**** FOUND 08:49:56.36 +14:48:30.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78774_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 78774_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
**** FOUND 08:42:55.59 +14:05:55.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78798_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 78798_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
**** FOUND 09:03:45.14 +09:54:14.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 78818_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 78818_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 78908_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 78908_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 78965_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 78965_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
**** FOUND 08:43:52.58 +10:16:00.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 79153_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 79153_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
**** FOUND 08:54:31.11 +15:35:55.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 2.169 609109826673273088 133.62914696938 +15.59827804826 14.0013 13.3470 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.169#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79168_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 79168_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 79225_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 79225_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 79261_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 79261_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
**** FOUND 08:45:55.29 +11:26:04.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 79525_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 79525_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 79547_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 79547_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 79713_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 79713_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
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Considering the candidate 79722_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 79722_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
**** FOUND 08:42:54.06 +10:21:35.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)GAIADR2_OUTPUT=# 0.752 598385877450353920 130.72506041309 +10.35982279083 14.2960 13.8307 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.752#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 79841_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 79841_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 79947_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 79947_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 79988_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 79988_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 80034_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 80034_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
**** FOUND 08:50:29.62 +17:02:33.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 80039_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 80039_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 80072_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
Preparing report for the candidate 80072_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
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Considering the candidate 80121_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 80121_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 80168_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 80168_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (117.9") between the two second-epoch detections
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Considering the candidate 80186_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 80186_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (140.4") between the two second-epoch detections
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Considering the candidate 80206_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 80206_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (88.8") between the two second-epoch detections
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Considering the candidate 80275_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 80275_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 80291_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
Preparing report for the candidate 80291_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
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Considering the candidate 80313_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 80313_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (124.3") between the two second-epoch detections
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Considering the candidate 80319_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 80319_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 80326_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 80326_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (107.3") between the two second-epoch detections
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Considering the candidate 80342_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 80342_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (192.8") between the two second-epoch detections
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Considering the candidate 80414_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 80414_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 80447_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 80447_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
**** FOUND 08:48:34.51 +10:23:07.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.61, MAG_FAINT_SEARCH_LIMIT=15.59)GAIADR2_OUTPUT=# 1.424 598526821097202944 132.14345907686 +10.38505561185 14.4812 13.8501 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.424#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 80500_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 80500_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 80559_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 80559_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 80564_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 80564_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 80566_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 80566_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (137.7") between the two second-epoch detections
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Considering the candidate 80577_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 80577_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (62.1") between the two second-epoch detections
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Considering the candidate 80580_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 80580_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (154.3") between the two second-epoch detections
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Considering the candidate 80584_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 80584_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
**** FOUND 09:00:45.78 +16:08:46.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.73, MAG_FAINT_SEARCH_LIMIT=15.71)GAIADR2_OUTPUT=# 2.970 610677249217995648 135.19141992352 +16.14679415253 14.8429 14.2731 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.970#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 80587_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 80587_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 80590_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 80590_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 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 80608_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 80608_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 80613_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345
The candidate 80613_fd_Cnc-05-Q2b1x1_2026-03-25_22-36-06_20.00sec_-10.00C_LIGHT_0345 did not pass the final checks