This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 27.1328* 05 28 14.82 +01 38 50.4 14.1 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461126.6328,14.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260327.1328 14.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:28:14.82 +01:38:50.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20_00sec_-14_90C_LIGHT_0149_fits__*pix.png resample_wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20_00sec_-10_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20_00sec_-14_90C_LIGHT_0149_fits__*pix.png resample_wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20_00sec_-10_00C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20_00sec_-14_90C_LIGHT_0149_fits__*pix.png resample_wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20_00sec_-10_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20_00sec_-14_90C_LIGHT_0149_fits__*pix.png resample_wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20_00sec_-10_00C_LIGHT_0076_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!
TCP 2026 03 27.1328* 04 57 54.03 -03 07 51.8 14.2 U Ori 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461126.6328,14.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260327.1328 14.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:57:54.03 -03:07:51.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20_00sec_-14_90C_LIGHT_0149_fits__*pix.png resample_wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20_00sec_-10_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20_00sec_-14_90C_LIGHT_0149_fits__*pix.png resample_wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20_00sec_-10_00C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20_00sec_-14_90C_LIGHT_0149_fits__*pix.png resample_wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20_00sec_-10_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20_00sec_-14_90C_LIGHT_0149_fits__*pix.png resample_wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20_00sec_-10_00C_LIGHT_0076_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!
TCP 2026 03 27.1328* 04 44 55.09 -01 25 44.9 14.2 U Eri 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461126.6328,14.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260327.1328 14.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:44:55.09 -01:25:44.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20_00sec_-14_90C_LIGHT_0149_fits__*pix.png resample_wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20_00sec_-10_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20_00sec_-14_90C_LIGHT_0149_fits__*pix.png resample_wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20_00sec_-10_00C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20_00sec_-14_90C_LIGHT_0149_fits__*pix.png resample_wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20_00sec_-10_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20_00sec_-14_90C_LIGHT_0149_fits__*pix.png resample_wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20_00sec_-10_00C_LIGHT_0076_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.68062513 09.01.2026 04:19:56.011 /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits
First image: 2461049.68062513 09.01.2026 04:19:56.011 /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits
Last image: 2461126.63309605 27.03.2026 03:11:29.499 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.68
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 12480
Objects passed selection criteria: 12415
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 9066.5
Average stars matched: 8551.75 (94.3225 %)
Memory usage VmPeak: 117712 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 Thu Mar 26 22:20:53 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461049.68062513 09.01.2026 04:19:56.011 /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits
First image: 2461049.68062513 09.01.2026 04:19:56.011 /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits
Last image: 2461126.63309605 27.03.2026 03:11:29.499 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 78
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.34
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: 16 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): 75227
Objects passed selection criteria: 75018
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 2.0 2 4
Average stars detected per image: 57359.8
Average stars matched: 54430.5 (94.8932 %)
Memory usage VmPeak: 173220 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 Thu Mar 26 22:21:57 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/Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits
SExtractor catalog cache: saved Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits.cat to cache
SExtractor catalog cache: saved Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.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/Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.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: 2461126.63259418
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Plate-solving the images
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits exists and is non-empty
Saving wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits to local_wcs_cache/
'wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits' -> 'local_wcs_cache/wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits'
wcs_Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits exists and is non-empty
Saving wcs_Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits to local_wcs_cache/
'wcs_Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits' -> 'local_wcs_cache/wcs_Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits'
wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits exists and is non-empty
Saving wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits to local_wcs_cache/
'wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits' -> 'local_wcs_cache/wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits'
wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits exists and is non-empty
Saving wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits to local_wcs_cache/
'wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits' -> 'local_wcs_cache/wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.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 05:08:40.809 -01:58:40.45
Second-epoch image center 05:08:47.236 -01:58:55.70
Angular distance between the image centers 0.03 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 05:08:40.809 -01:58:40.45
Second-epoch image center 05:08:46.853 -01:58:54.48
Angular distance between the image centers 0.03 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 05:08:47.236 -01:58:55.70
Second-epoch second image center 05:08:46.853 -01:58:54.48
Angular distance between the image centers 0.00163 deg.
###################################
ERROR: no shift applied between second-epoch images! The distance between image centers is 0.00163 deg. (min. required shift: 0.00164 deg.)
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits &> /tmp/tmp.P6bbUoQfG5
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits &> /tmp/tmp.Cil25pQOeS
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits &> /tmp/tmp.nXYvflcm06
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits &> /tmp/tmp.QDgtFYH6Nq
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits
Calibrating the magnitude scale
Found non-empty wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.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_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits and wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.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_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits and wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits.cat
Found non-empty wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits and wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits.cat
The reference image (wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits) and catalog (wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits.cat) found
'wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.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 7990 out of 14462 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.902554
a=0.000000 b=1.000000 c=22.902554
From vast_summary.log: estimated ref. image limiting mag.: -7.68
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.22
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.22
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits
2.1 pix Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits
2.6 pix fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits
2.6 pix fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits
Limiting magnitude estimates:
15.2 mag. Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits
15.2 mag. Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits
14.1 mag. fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits
14.1 mag. fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 11.2 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.P6bbUoQfG5 (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/Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.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_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits' -> 'wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits
WCS_IMAGE_NAME=wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits
WCS-calibrated image found: wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits
Checking if the catalog wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits.cat corresponding to the image wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits alredy exist and is non-empty...
Catalog wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits.cat corresponding to the image wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits
WCS catalog name: wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1502, passed=14462
Got 14462 stars (including 12945 good ones) from the SExtractor catalog wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits.cat
util/solve_plate_with_UCAC5 got 14462 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.35"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 932 stars left (next iteration limit 1025)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits -region wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.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.Cil25pQOeS (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/Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.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_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits' -> 'wcs_Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits
WCS_IMAGE_NAME=wcs_Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits
WCS-calibrated image found: wcs_Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits
Checking if the catalog wcs_Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits.cat corresponding to the image wcs_Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits alredy exist and is non-empty...
Catalog wcs_Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits.cat corresponding to the image wcs_Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits
WCS catalog name: wcs_Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=1458, passed=14500
Got 14500 stars (including 13020 good ones) from the SExtractor catalog wcs_Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits.cat
util/solve_plate_with_UCAC5 got 14500 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
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 930 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 929 stars left (next iteration limit 1021)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits -region wcs_Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.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.nXYvflcm06 (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_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.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_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits
WCS_IMAGE_NAME=wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits
WCS-calibrated image found: wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits
Checking if the catalog wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits.cat corresponding to the image wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits.cat corresponding to the image wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits
WCS catalog name: wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=694, passed=7113
Got 7113 stars (including 6412 good ones) from the SExtractor catalog wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits.cat
util/solve_plate_with_UCAC5 got 7113 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 925 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: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.51"
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 925 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.51"
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 923 stars left (next iteration limit 1015)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits -region wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.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.QDgtFYH6Nq (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_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.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_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits
WCS_IMAGE_NAME=wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits
WCS-calibrated image found: wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits
Checking if the catalog wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits.cat corresponding to the image wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits.cat corresponding to the image wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits
WCS catalog name: wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=685, passed=7111
Got 7111 stars (including 6419 good ones) from the SExtractor catalog wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits.cat
util/solve_plate_with_UCAC5 got 7111 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 922 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: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.51"
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 922 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.51"
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 919 stars left (next iteration limit 1010)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits -region wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.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_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits'
Saving fully-calibrated image wcs_Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/wcs_Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits'
Saving fully-calibrated image wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits'
Saving fully-calibrated image wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits'
Preparing the HTML report for the field Ori-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
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 21453_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 21453_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:24:34.46 -02:22:38.1 in the exclusion list exclusion_list_bbsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Ori-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/Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits
SExtractor catalog cache: saved Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits.cat to cache
SExtractor catalog cache: saved Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits
Creating symlink local_wcs_cache/wcs_Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits
Creating symlink local_wcs_cache/wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits
Creating symlink local_wcs_cache/wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.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_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits exists and is non-empty
wcs_Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits exists and is non-empty
wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits exists and is non-empty
wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.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 05:08:40.809 -01:58:40.45
Second-epoch image center 05:08:47.236 -01:58:55.70
Angular distance between the image centers 0.03 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 05:08:40.809 -01:58:40.45
Second-epoch image center 05:08:46.853 -01:58:54.48
Angular distance between the image centers 0.03 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 05:08:47.236 -01:58:55.70
Second-epoch second image center 05:08:46.853 -01:58:54.48
Angular distance between the image centers 0.00163 deg.
###################################
ERROR: no shift applied between second-epoch images! The distance between image centers is 0.00163 deg. (min. required shift: 0.00164 deg.)
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits &> /tmp/tmp.RSFQ5cZ6zW
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits &> /tmp/tmp.pJpaD8qudc
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits &> /tmp/tmp.ozQ9CVV9X6
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits &> /tmp/tmp.x7RyIMKmX4
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits
Calibrating the magnitude scale
Found non-empty wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.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_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits and wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.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_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits and wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits.cat
Found non-empty wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits and wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits.cat
The reference image (wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits) and catalog (wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits.cat) found
'wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.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 8155 out of 88009 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.769707
a=0.000000 b=1.000000 c=22.769707
From vast_summary.log: estimated ref. image limiting mag.: -7.34
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.43
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.43
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 60 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits
1.9 pix Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits
2.2 pix fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits
2.2 pix fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits
Limiting magnitude estimates:
15.4 mag. Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits
15.4 mag. Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits
14.2 mag. fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits
14.2 mag. fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits
All-image limiting magnitude estimate: 14.2 (SNR ) 13.8 (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.RSFQ5cZ6zW (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/Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.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_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits' -> 'wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits
WCS_IMAGE_NAME=wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits
WCS-calibrated image found: wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits
Checking if the catalog wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits.cat corresponding to the image wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits alredy exist and is non-empty...
Catalog wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits.cat corresponding to the image wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits
WCS catalog name: wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=24, blended=6760, passed=87985
Got 87985 stars (including 81076 good ones) from the SExtractor catalog wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits.cat
util/solve_plate_with_UCAC5 got 87985 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
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 937 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: 0.34"
Excluding outliers - 935 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits -region wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.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.pJpaD8qudc (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/Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.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_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits' -> 'wcs_Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits
WCS_IMAGE_NAME=wcs_Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits
WCS-calibrated image found: wcs_Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits
Checking if the catalog wcs_Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits.cat corresponding to the image wcs_Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits alredy exist and is non-empty...
Catalog wcs_Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits.cat corresponding to the image wcs_Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits
WCS catalog name: wcs_Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=26, blended=6799, passed=87254
Got 87254 stars (including 80318 good ones) from the SExtractor catalog wcs_Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits.cat
util/solve_plate_with_UCAC5 got 87254 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
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 935 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: 0.34"
Excluding outliers - 933 stars left (next iteration limit 1026)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits -region wcs_Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.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.ozQ9CVV9X6 (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_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.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_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits
WCS_IMAGE_NAME=wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits
WCS-calibrated image found: wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits
Checking if the catalog wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits.cat corresponding to the image wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits.cat corresponding to the image wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits
WCS catalog name: wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=2348, passed=42932
Got 42932 stars (including 40535 good ones) from the SExtractor catalog wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits.cat
util/solve_plate_with_UCAC5 got 42932 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 926 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.52"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 926 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.52"
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 922 stars left (next iteration limit 1014)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits -region wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.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.x7RyIMKmX4 (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_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.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_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits
WCS_IMAGE_NAME=wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits
WCS-calibrated image found: wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits
Checking if the catalog wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits.cat corresponding to the image wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits alredy exist and is non-empty...
Catalog wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits.cat corresponding to the image wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits
WCS catalog name: wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=2314, passed=42488
Got 42488 stars (including 40116 good ones) from the SExtractor catalog wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits.cat
util/solve_plate_with_UCAC5 got 42488 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (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 0.010417 (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 924 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.52"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 924 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.52"
Estimated accuracy of the plate solution: 0.52"
Excluding outliers - 920 stars left (next iteration limit 1012)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits -region wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.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_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.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_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/wcs_Ori-05-Q2b1x1_2026-01-08_22-19-56_20.00sec_-14.90C_LIGHT_0149.fits
Saving fully-calibrated image wcs_Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.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_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/wcs_Ori-05-Q2b1x1_2026-01-08_22-21-00_20.00sec_-14.90C_LIGHT_0150.fits
Saving fully-calibrated image wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.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_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-10-46_20.00sec_-10.00C_LIGHT_0076.fits
Saving fully-calibrated image wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.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_2026-03-26_CI_Ori-05-Q2b1x1_221836_TTUQ2b1x1_25698_Vo3h5G0S/wcs_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077.fits
Preparing the HTML report for the field Ori-05-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out103730.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103734.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103739.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103741.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103743.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107529.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out107959.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out108074.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out109105.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out109201.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out109054.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out109136.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out109187.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 15s
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 103722_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 103722_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:10:36.20 -02:21:05.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103727_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 103727_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:07:23.60 -00:49:11.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103730_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 103730_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:55:59.88 +00:41:49.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 0.236 3228473560026122752 073.99956504507 +00.69712019918 13.2528 12.5782 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.236#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103734_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 103734_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:14:20.98 +01:51:52.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 2.700 3234093404474892928 078.58679184257 +01.86408451602 13.7550 13.2473 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.700#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103737_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 103737_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:59:46.52 +01:52:56.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103739_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 103739_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:26:36.87 -02:54:04.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.95, MAG_FAINT_SEARCH_LIMIT=13.93)
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Considering the candidate 103741_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 103741_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:11:52.52 +00:53:40.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)GAIADR2_OUTPUT=# 2.370 3233886696288641920 077.96829015742 +00.89432220000 13.0639 12.6690 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.370#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103743_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 103743_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:58:10.87 +01:31:52.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 1.087 3231922281326461184 074.54501550999 +01.53137221626 12.8684 12.1440 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.087#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103745_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 103745_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:07:27.59 -00:32:41.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 104766_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 104766_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:24:22.83 -02:25:55.0 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 105173_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 105173_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 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 105520_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 105520_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 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 106094_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 106094_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:13:27.83 +01:56:09.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 106130_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 106130_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 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 106179_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 106179_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:50:40.71 -04:07:13.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106262_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 106262_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:09:56.57 -00:33:21.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 106381_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 106381_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:25:27.38 -00:33:54.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 106409_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 106409_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 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 106813_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 106813_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:11:43.19 +00:29:25.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 106847_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 106847_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:00:46.04 -02:04:49.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 106884_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 106884_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:55:58.35 +01:36:16.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 106897_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 106897_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:58:06.83 -02:13:55.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 106935_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 106935_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 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 107459_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 107459_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 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 107529_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 107529_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:11:00.75 -01:46:21.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 3.147 3214916375497054720 077.75396502823 -01.77296601833 13.3532 12.8894 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.147#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 107568_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 107568_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 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 107629_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 107629_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:58:06.25 -02:13:20.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 107633_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 107633_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 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 107637_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 107637_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 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 107867_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 107867_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 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 107879_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 107879_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 04:58:41.36 +01:42:38.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 107959_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 107959_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:08:27.09 -01:31:54.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 4.155 3214994165944608896 077.11177027787 -01.53133103285 13.9994 13.4868 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.155#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 108027_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 108027_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:16:31.95 -05:02:55.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 108053_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 108053_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 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 108074_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 108074_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:05:25.72 -03:28:35.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 1.247 3212995356884864512 076.35706413571 -03.47614126517 13.3976 12.7949 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.247#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 108217_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 108217_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:11:46.67 -00:40:11.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 108252_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 108252_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 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 108297_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 108297_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 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 108422_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 108422_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:14:10.06 +01:28:51.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 108733_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 108733_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 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 108775_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 108775_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 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 108778_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 108778_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 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 108803_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 108803_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 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 108912_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 108912_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 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 108941_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 108941_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 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 108954_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 108954_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 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 108955_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 108955_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:00:39.44 -00:10:44.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 108987_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 108987_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 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 109054_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
Preparing report for the candidate 109054_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
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Considering the candidate 109105_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 109105_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:08:32.90 -01:33:02.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)GAIADR2_OUTPUT=# 1.061 3214991142287632128 077.13699810990 -01.55108768954 14.4294 13.8843 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.061#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 109136_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
Preparing report for the candidate 109136_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
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Considering the candidate 109141_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 109141_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 109165_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 109165_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 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 109180_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 109180_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 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 109187_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
Preparing report for the candidate 109187_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
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Considering the candidate 109201_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 109201_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:08:52.17 -01:14:53.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 2.279 3227014851693789184 077.21674297999 -01.24828917740 14.1792 13.4998 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.279#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 109202_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 109202_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 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 109209_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 109209_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 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 109217_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 109217_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 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 109223_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077
The candidate 109223_fd_Ori-05-Q2b1x1_2026-03-26_22-11-29_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks