This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461129.6551,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260330.1551 13.12CV 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/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:17:37.64 +35:09:58.4 ;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_Aur-04-Q2b1x1_2026-01-20_23-14-47_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20_00sec_-10_00C_LIGHT_0119_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20_00sec_-10_00C_LIGHT_0118_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20_00sec_-10_00C_LIGHT_0119_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20_00sec_-10_00C_LIGHT_0118_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461129.6551,13.18,0.05,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 20260330.1551 13.18CV 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/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:17:45.08 +40:23:27.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20_00sec_-10_00C_LIGHT_0119_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20_00sec_-10_00C_LIGHT_0118_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20_00sec_-10_00C_LIGHT_0119_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20_00sec_-10_00C_LIGHT_0118_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0608537+363513,2461129.6551,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0608537+363513 20260330.1551 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:08:53.76 +36:35:08.8 ;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_Aur-04-Q2b1x1_2026-01-20_23-14-47_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20_00sec_-10_00C_LIGHT_0119_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20_00sec_-10_00C_LIGHT_0118_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20_00sec_-10_00C_LIGHT_0119_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20_00sec_-15_00C_LIGHT_0232_fits__*pix.png resample_wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20_00sec_-10_00C_LIGHT_0118_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: 2461061.71871545 21.01.2026 05:14:47.015 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
First image: 2461061.71871545 21.01.2026 05:14:47.015 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
Last image: 2461129.65550369 30.03.2026 03:43:45.519 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.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.: -7.64
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: 6 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): 19411
Objects passed selection criteria: 19298
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 13636.5
Average stars matched: 13005 (95.369 %)
Memory usage VmPeak: 124040 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Mar 29 22:47:22 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: 2461061.71871545 21.01.2026 05:14:47.015 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
First image: 2461061.71871545 21.01.2026 05:14:47.015 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
Last image: 2461129.65550369 30.03.2026 03:43:45.519 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 69
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.30
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: 121 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): 139456
Objects passed selection criteria: 139072
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 100750
Average stars matched: 95208.2 (94.4995 %)
Memory usage VmPeak: 1966388 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Mar 29 22:51:38 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/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits
SExtractor catalog cache: saved Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat to cache
SExtractor catalog cache: saved Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.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/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461129.65478991
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits exists and is non-empty
Saving wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits to local_wcs_cache/
'wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits' -> 'local_wcs_cache/wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits'
wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits exists and is non-empty
Saving wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits to local_wcs_cache/
'wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits' -> 'local_wcs_cache/wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits'
wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits exists and is non-empty
Saving wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits to local_wcs_cache/
'wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits' -> 'local_wcs_cache/wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits'
wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits exists and is non-empty
Saving wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits to local_wcs_cache/
'wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits' -> 'local_wcs_cache/wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.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 06:32:43.667 +37:59:56.47
Second-epoch image center 06:32:46.337 +37:59:46.63
Angular distance between the image centers 0.01 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 06:32:43.667 +37:59:56.47
Second-epoch image center 06:32:48.530 +38:00:18.84
Angular distance between the image centers 0.02 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 06:32:46.337 +37:59:46.63
Second-epoch second image center 06:32:48.530 +38:00:18.84
Angular distance between the image centers 0.01149 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/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits &> /tmp/tmp.nklQdXf1Yv
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits &> /tmp/tmp.D12X9XuLEJ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits &> /tmp/tmp.IQ45tEa54A
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits &> /tmp/tmp.8S3ZQpRCrT
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.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_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.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_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat
Found non-empty wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat
The reference image (wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits) and catalog (wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat) found
'wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.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 11206 out of 22646 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.938798
a=0.000000 b=1.000000 c=22.938798
From vast_summary.log: estimated ref. image limiting mag.: -7.64
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.30
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.30
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
2.0 pix Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
2.6 pix fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits
2.6 pix fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits
Limiting magnitude estimates:
15.3 mag. Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
15.3 mag. Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
14.1 mag. fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits
14.2 mag. fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 11.4 (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.nklQdXf1Yv (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/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits' -> 'wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
WCS_IMAGE_NAME=wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
WCS-calibrated image found: wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
Checking if the catalog wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat corresponding to the image wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits alredy exist and is non-empty...
Catalog wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat corresponding to the image wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
WCS catalog name: wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2024, passed=22646
Got 22646 stars (including 20590 good ones) from the SExtractor catalog wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat
util/solve_plate_with_UCAC5 got 22646 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.32"
Estimated accuracy of the plate solution: 0.33"
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_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits -region wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.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.D12X9XuLEJ (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/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits' -> 'wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
WCS_IMAGE_NAME=wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
WCS-calibrated image found: wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
Checking if the catalog wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat corresponding to the image wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits alredy exist and is non-empty...
Catalog wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat corresponding to the image wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
WCS catalog name: wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2057, passed=22538
Got 22538 stars (including 20456 good ones) from the SExtractor catalog wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat
util/solve_plate_with_UCAC5 got 22538 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.35"
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 937 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: 0.35"
Excluding outliers - 934 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits -region wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.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.IQ45tEa54A (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits
WCS_IMAGE_NAME=wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits
WCS-calibrated image found: wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits
Checking if the catalog wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits.cat corresponding to the image wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits.cat corresponding to the image wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits
WCS catalog name: wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=584, passed=9397
Got 9397 stars (including 8803 good ones) from the SExtractor catalog wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits.cat
util/solve_plate_with_UCAC5 got 9397 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 927 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: 0.70"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.68"
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 927 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.69"
Estimated accuracy of the plate solution: 0.75"
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_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits -region wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.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.8S3ZQpRCrT (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits
WCS_IMAGE_NAME=wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits
WCS-calibrated image found: wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits
Checking if the catalog wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits.cat corresponding to the image wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits.cat corresponding to the image wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits
WCS catalog name: wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=578, passed=9537
Got 9537 stars (including 8950 good ones) from the SExtractor catalog wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits.cat
util/solve_plate_with_UCAC5 got 9537 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 927 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: 0.69"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.67"
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 927 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.68"
Estimated accuracy of the plate solution: 0.74"
Excluding outliers - 924 stars left (next iteration limit 1016)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits -region wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.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_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits'
Saving fully-calibrated image wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits'
Saving fully-calibrated image wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits'
Saving fully-calibrated image wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits'
Preparing the HTML report for the field Aur-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32237_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 32237_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks
**** FOUND 06:28:01.82 +36:04:59.6 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 0s
Prepared the HTML report for the field Aur-04-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/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits
SExtractor catalog cache: saved Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat to cache
SExtractor catalog cache: saved Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
Creating symlink local_wcs_cache/wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.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_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits exists and is non-empty
wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits exists and is non-empty
wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits exists and is non-empty
wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.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 06:32:43.667 +37:59:56.47
Second-epoch image center 06:32:46.337 +37:59:46.63
Angular distance between the image centers 0.01 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 06:32:43.667 +37:59:56.47
Second-epoch image center 06:32:48.530 +38:00:18.84
Angular distance between the image centers 0.02 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 06:32:46.337 +37:59:46.63
Second-epoch second image center 06:32:48.530 +38:00:18.84
Angular distance between the image centers 0.01149 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/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits &> /tmp/tmp.F0jAgUp1s0
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits &> /tmp/tmp.YOguH0X8N0
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits &> /tmp/tmp.Lib0Jwnw2e
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits &> /tmp/tmp.6aik1Cr66i
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.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_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.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_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat
Found non-empty wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat
The reference image (wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits) and catalog (wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat) found
'wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.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 11458 out of 160824 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.781706
a=0.000000 b=1.000000 c=22.781706
From vast_summary.log: estimated ref. image limiting mag.: -7.30
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.48
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.48
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 56 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
1.9 pix Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
2.4 pix fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits
2.4 pix fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits
Limiting magnitude estimates:
15.5 mag. Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
15.5 mag. Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
14.2 mag. fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits
14.3 mag. fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits
All-image limiting magnitude estimate: 14.2 (SNR ) 13.7 (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.F0jAgUp1s0 (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/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits' -> 'wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
WCS_IMAGE_NAME=wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
WCS-calibrated image found: wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
Checking if the catalog wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat corresponding to the image wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits alredy exist and is non-empty...
Catalog wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat corresponding to the image wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
WCS catalog name: wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=32, blended=18360, passed=160792
Got 160792 stars (including 142160 good ones) from the SExtractor catalog wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat
util/solve_plate_with_UCAC5 got 160792 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
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: 0.37"
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 928 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_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits -region wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.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.YOguH0X8N0 (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/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits' -> 'wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
WCS_IMAGE_NAME=wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
WCS-calibrated image found: wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
Checking if the catalog wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat corresponding to the image wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits alredy exist and is non-empty...
Catalog wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat corresponding to the image wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
WCS catalog name: wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=25, blended=18627, passed=162444
Got 162444 stars (including 143508 good ones) from the SExtractor catalog wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat
util/solve_plate_with_UCAC5 got 162444 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.39"
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 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_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits -region wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.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.Lib0Jwnw2e (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits
WCS_IMAGE_NAME=wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits
WCS-calibrated image found: wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits
Checking if the catalog wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits.cat corresponding to the image wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits.cat corresponding to the image wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits
WCS catalog name: wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=4098, passed=63709
Got 63709 stars (including 59555 good ones) from the SExtractor catalog wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits.cat
util/solve_plate_with_UCAC5 got 63709 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.70"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.64"
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: 0.64"
Estimated accuracy of the plate solution: 0.71"
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_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits -region wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.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.6aik1Cr66i (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits
WCS_IMAGE_NAME=wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits
WCS-calibrated image found: wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits
Checking if the catalog wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits.cat corresponding to the image wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits.cat corresponding to the image wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits
WCS catalog name: wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=3973, passed=63362
Got 63362 stars (including 59323 good ones) from the SExtractor catalog wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits.cat
util/solve_plate_with_UCAC5 got 63362 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 921 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: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.63"
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 921 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.63"
Estimated accuracy of the plate solution: 0.68"
Excluding outliers - 918 stars left (next iteration limit 1009)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits -region wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.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_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
Saving fully-calibrated image wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
Saving fully-calibrated image wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-42-43_20.00sec_-10.00C_LIGHT_0118.fits
Saving fully-calibrated image wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-04-Q2b1x1_224502_TTUQ2b1x1_29697_NohkFmcJ/wcs_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119.fits
Preparing the HTML report for the field Aur-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out171468.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out184300.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out184305.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out184307.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out184313.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out184318.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out184319.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out184322.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out184325.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out184327.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out184328.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out185994.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out186187.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out186357.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out187093.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out187793.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out187836.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out187889.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out187909.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out188260.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out188286.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out188475.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out188573.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out188578.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out188597.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out188655.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out188691.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out188800.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out189078.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out189109.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out189222.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out189261.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out189616.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out189690.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out189957.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out190306.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out190335.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out190511.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out190543.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out190573.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out190728.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out191373.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out191559.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out191696.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out192256.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out85457.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out189001.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out189410.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out67916.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 17s
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 184300_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 184300_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks
**** FOUND 06:52:59.78 +39:28:32.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 1.396 944537014325667968 103.24888117252 +39.47536717175 13.8426 13.2908 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.396#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 184305_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 184305_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks
**** FOUND 06:58:11.51 +37:56:35.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 1.729 941160929513585408 104.54734939614 +37.94328865841 13.7611 13.2199 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.729#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 184307_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 184307_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks
**** FOUND 06:26:44.66 +40:51:20.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)
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Considering the candidate 184313_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 184313_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks
**** FOUND 06:28:43.06 +35:47:30.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 5.567 942614861841932416 097.18051704043 +35.79065395643 13.7656 13.1853 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.567#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 184318_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 184318_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks
**** FOUND 06:51:17.92 +38:00:56.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 0.549 944127716826675072 102.82483116596 +38.01566377495 13.4663 12.9662 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.549#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 184319_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 184319_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks
**** FOUND 06:33:06.14 +34:09:32.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 0.536 941579465486722048 098.27549102210 +34.15895559206 13.4719 12.9850 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.536#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 184322_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 184322_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks
**** FOUND 06:14:22.66 +39:06:53.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 3.128 956291201647574528 093.59553555279 +39.11488112300 13.4663 12.9811 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.128#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 184325_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 184325_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks
**** FOUND 06:38:19.28 +35:49:22.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 0.370 942160729179818240 099.58041209894 +35.82291933815 13.0188 12.2415 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.370#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 184327_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 184327_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks
**** FOUND 07:01:19.47 +38:16:51.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 1.381 947008338507875456 105.33106581804 +38.28059137287 13.1172 12.5943 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.381#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 184328_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 184328_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks
**** FOUND 06:19:41.69 +41:03:47.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)
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Considering the candidate 185994_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 185994_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks
**** FOUND 06:57:10.58 +37:22:27.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.99, MAG_FAINT_SEARCH_LIMIT=12.97)GAIADR2_OUTPUT=# 0.756 940932810914155136 104.29416160612 +37.37402161757 11.9547 11.5814 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.756#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 186187_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 186187_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks
**** FOUND 06:09:09.87 +34:55:02.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.03, MAG_FAINT_SEARCH_LIMIT=13.01)GAIADR2_OUTPUT=# 0.267 3452521349359078784 092.29108636410 +34.91732177152 11.7973 11.0372 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.267#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 186357_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 186357_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks
**** FOUND 06:57:29.11 +37:23:35.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 0.524 940932334174069504 104.37144967043 +37.39317608856 12.1122 11.7116 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.524#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 187093_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 187093_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks
**** FOUND 06:13:27.56 +37:08:30.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 1.464 3453919760648422912 093.36491566555 +37.14151522618 12.2112 11.4278 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.464#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 187793_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 187793_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks
**** FOUND 06:15:09.00 +39:55:26.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.69, MAG_FAINT_SEARCH_LIMIT=13.67)GAIADR2_OUTPUT=# 1.196 959420622196433024 093.78757593139 +39.92358963702 12.6142 12.1045 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.196#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 187836_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 187836_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks
**** FOUND 06:18:45.87 +38:13:35.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 1.920 956048931132973696 094.69178721095 +38.22627193678 12.8536 12.4158 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.920#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 187889_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 187889_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks
**** FOUND 06:16:12.83 +37:38:42.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 1.817 955914103518773248 094.05394938237 +37.64532186433 12.8175 12.5622 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.817#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 187909_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 187909_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks
**** FOUND 06:50:16.33 +36:25:14.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 0.066 940630518230727296 102.56802720735 +36.42079149688 12.8853 12.4563 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.066#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 188260_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 188260_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks
**** FOUND 06:08:27.81 +35:09:27.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 4.122 3453282383204191104 092.11449733715 +35.15792799607 12.7110 11.8583 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.122#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 188286_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 188286_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks
**** FOUND 06:59:55.16 +36:55:53.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 2.161 940847323884747776 104.97917694125 +36.93131977308 13.1391 12.4971 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.161#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 188475_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 188475_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks
**** FOUND 06:17:37.67 +35:07:37.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 5.763 3452639482436245504 094.40863227678 +35.12802388446 12.8262 12.0796 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.763#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 188573_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 188573_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks
**** FOUND 06:24:45.72 +35:16:03.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.94, MAG_FAINT_SEARCH_LIMIT=13.92)GAIADR2_OUTPUT=# 0.579 942679114553730176 096.19069537010 +35.26756334742 12.6377 11.7487 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.579#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 188578_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 188578_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks
**** FOUND 06:50:17.56 +35:04:48.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 1.109 940236480752979328 102.57353978926 +35.08004089278 13.1897 12.9241 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.109#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 188597_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 188597_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks
**** FOUND 06:17:39.40 +39:49:59.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.00, MAG_FAINT_SEARCH_LIMIT=13.98)GAIADR2_OUTPUT=# 1.366 956429160294119808 094.41429103472 +39.83285506748 12.8257 12.0413 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.366#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 188655_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 188655_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks
**** FOUND 06:48:29.65 +39:33:02.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 2.067 944585117959343744 102.12282540988 +39.55085159646 13.1667 12.7358 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.067#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 188691_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 188691_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks
**** FOUND 06:30:53.88 +39:45:26.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 1.536 957304710850184448 097.72461351985 +39.75691580808 13.0948 12.5916 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.536#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 188784_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 188784_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks
**** FOUND 06:50:56.98 +41:46:51.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 188800_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 188800_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks
**** FOUND 06:09:00.39 +34:55:06.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 5.135 3452524235577101568 092.24998740495 +34.91900886294 12.7974 11.8492 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.135#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 189001_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
Preparing report for the candidate 189001_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
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Considering the candidate 189078_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 189078_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks
**** FOUND 06:13:49.41 +36:58:55.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 0.748 3453870351344674048 093.45609569195 +36.98230430743 12.9902 12.5363 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.748#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 189109_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 189109_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks
**** FOUND 06:18:08.09 +35:34:33.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 4.683 3452790905803337216 094.53530721163 +35.57594767215 13.2209 12.5875 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.683#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 189222_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 189222_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks
**** FOUND 06:55:32.16 +40:06:58.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 0.785 950585496509595136 103.88428522166 +40.11619542511 13.0248 12.3261 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.785#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 189223_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 189223_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks
**** FOUND 06:50:56.38 +41:47:33.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 189261_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 189261_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks
**** FOUND 06:59:00.59 +39:47:30.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 1.691 950408814438828288 104.75266895703 +39.79221871843 13.0918 12.4256 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.691#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 189410_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
Preparing report for the candidate 189410_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
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Considering the candidate 189616_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 189616_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks
**** FOUND 06:41:05.17 +34:14:23.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 2.923 938803885821606528 100.27252390345 +34.23978362340 13.5734 13.0794 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.923#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 189690_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 189690_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks
**** FOUND 06:44:45.71 +38:45:40.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)GAIADR2_OUTPUT=# 1.459 945194350481770368 101.18996516164 +38.76106608891 13.3419 12.8177 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.459#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 189957_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 189957_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks
**** FOUND 06:53:56.52 +36:31:34.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 1.260 940785446292643328 103.48511516696 +36.52594696103 13.6445 13.1079 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.260#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 190306_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 190306_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks
**** FOUND 06:56:57.28 +39:51:14.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 2.730 950380471950238976 104.23800539428 +39.85338122705 13.3802 12.6292 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.730#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 190335_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 190335_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks
**** FOUND 06:41:04.43 +34:19:29.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 3.865 938816530205315712 100.26973753110 +34.32461475584 13.9480 13.3723 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.865#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 190511_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 190511_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks
**** FOUND 06:36:11.72 +37:59:28.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 3.027 943411698535480192 099.04777322907 +37.99126064598 13.6137 12.9001 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.027#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 190543_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 190543_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks
**** FOUND 06:28:04.41 +36:10:59.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 0.220 942828785574237184 097.01844758965 +36.18312154877 13.2973 12.5291 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.220#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 190573_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 190573_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks
**** FOUND 06:46:26.79 +40:16:04.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 2.185 945430676761879168 101.61106332053 +40.26748699687 13.6422 12.9283 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.185#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 190728_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 190728_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks
**** FOUND 06:38:14.29 +42:00:40.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 1.012 958005894327207424 099.55991898990 +42.01131358101 13.4130 13.0135 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.012#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 191373_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 191373_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks
**** FOUND 06:40:14.63 +34:55:19.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 1.611 941871351464372352 100.06041299606 +34.92206473848 13.8912 13.2856 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.611#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 191443_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 191443_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks
**** FOUND 06:52:52.64 +38:52:34.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 191559_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 191559_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks
**** FOUND 06:51:24.49 +38:34:43.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 0.594 944296594940449536 102.85187554182 +38.57859258613 13.7030 13.2329 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.594#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 191696_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 191696_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks
**** FOUND 06:33:09.41 +37:34:18.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 4.025 943384760500759168 098.29061532632 +37.57191475343 14.0283 13.7779 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.025#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 192256_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 192256_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks
**** FOUND 06:50:18.72 +36:25:11.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.28, MAG_FAINT_SEARCH_LIMIT=15.26)GAIADR2_OUTPUT=# 2.611 940630896190029440 102.57881369946 +36.41957678465 14.1110 13.5358 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.611#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 53350_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 53350_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks
**** FOUND 06:28:01.88 +36:04:59.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 91158_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 91158_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks
**** FOUND 06:06:38.96 +37:57:56.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33022_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 33022_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks
**** FOUND 06:18:23.10 +34:38:16.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 67916_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
Preparing report for the candidate 67916_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
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Considering the candidate 127321_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 127321_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks
**** FOUND 06:15:48.75 +41:02:19.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 85457_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 85457_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks
**** FOUND 06:24:01.56 +37:59:29.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.69, MAG_FAINT_SEARCH_LIMIT=14.67)
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Considering the candidate 171468_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119
The candidate 171468_fd_Aur-04-Q2b1x1_2026-03-29_22-43-45_20.00sec_-10.00C_LIGHT_0119 did not pass the final checks