This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 29.1048* 05 14 06.75 +25 56 25.0 12.4 U Tau 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461128.6048,12.44,0.05,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 20260329.1048 12.44CV 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-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:14:06.75 +25:56:25.0 ;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-05-Q2b1x1_2026-02-11_20-25-42_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20_00sec_-10_00C_LIGHT_0031_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20_00sec_-10_00C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20_00sec_-10_00C_LIGHT_0031_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20_00sec_-10_00C_LIGHT_0030_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461128.6048,13.91,0.05,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 20260329.1048 13.91CV 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-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:20:25.60 +33:09:01.7 ;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-05-Q2b1x1_2026-02-11_20-25-42_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20_00sec_-10_00C_LIGHT_0031_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20_00sec_-10_00C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20_00sec_-10_00C_LIGHT_0031_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20_00sec_-10_00C_LIGHT_0030_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461128.6048,14.46,0.05,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 20260329.1048 14.46CV 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-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:29:01.45 +30:05:27.6 ;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-05-Q2b1x1_2026-02-11_20-25-42_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20_00sec_-10_00C_LIGHT_0031_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20_00sec_-10_00C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20_00sec_-10_00C_LIGHT_0031_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20_00sec_-10_00C_LIGHT_0030_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461128.6048,13.10,0.05,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 20260329.1048 13.10CV 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-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:29:39.94 +30:52:52.8 ;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-05-Q2b1x1_2026-02-11_20-25-42_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20_00sec_-10_00C_LIGHT_0031_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20_00sec_-10_00C_LIGHT_0030_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20_00sec_-10_00C_LIGHT_0031_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20_00sec_-10_00C_LIGHT_0030_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: 2461083.60130240 12.02.2026 02:25:42.527 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits
First image: 2461083.60130240 12.02.2026 02:25:42.527 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits
Last image: 2461128.60505312 29.03.2026 02:31:06.590 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 9
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.50
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 13283
Objects passed selection criteria: 13248
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 10824.8
Average stars matched: 10559.2 (97.5473 %)
Memory usage VmPeak: 119604 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 Sat Mar 28 21:37:10 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: 2461083.60130240 12.02.2026 02:25:42.527 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits
First image: 2461083.60130240 12.02.2026 02:25:42.527 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits
Last image: 2461128.60505312 29.03.2026 02:31:06.590 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 118
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.19
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: 32 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): 113312
Objects passed selection criteria: 113061
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 94203.8
Average stars matched: 91004.2 (96.6036 %)
Memory usage VmPeak: 1889360 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 Sat Mar 28 21:39:06 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-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits
SExtractor catalog cache: saved Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits.cat to cache
SExtractor catalog cache: saved Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.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-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.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: 2461128.60452631
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-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits exists and is non-empty
Saving wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits to local_wcs_cache/
'wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits' -> 'local_wcs_cache/wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits'
wcs_Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits exists and is non-empty
Saving wcs_Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits to local_wcs_cache/
'wcs_Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits' -> 'local_wcs_cache/wcs_Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits'
wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits exists and is non-empty
Saving wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits to local_wcs_cache/
'wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits' -> 'local_wcs_cache/wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits'
wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits exists and is non-empty
Saving wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits to local_wcs_cache/
'wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits' -> 'local_wcs_cache/wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:00:00.928 +29:59:47.56
Second-epoch image center 04:59:55.393 +29:56:10.02
Angular distance between the image centers 0.06 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:00:00.928 +29:59:47.56
Second-epoch image center 04:59:54.300 +29:56:16.19
Angular distance between the image centers 0.06 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 04:59:55.393 +29:56:10.02
Second-epoch second image center 04:59:54.300 +29:56:16.19
Angular distance between the image centers 0.00430 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-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits &> /tmp/tmp.eh2a5fvnJh
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits &> /tmp/tmp.PsWMIPd9lf
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits &> /tmp/tmp.GwKSwZhQjD
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits &> /tmp/tmp.pp4TqXYaQN
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.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-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits and wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.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-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits and wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits.cat
Found non-empty wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits and wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits.cat
The reference image (wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits) and catalog (wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits.cat) found
'wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.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 6737 out of 16419 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.972082
a=0.000000 b=1.000000 c=22.972082
From vast_summary.log: estimated ref. image limiting mag.: -7.50
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.47
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.47
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:
1.9 pix Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits
1.8 pix Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits
2.4 pix fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits
2.4 pix fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits
Limiting magnitude estimates:
15.5 mag. Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits
15.5 mag. Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits
14.6 mag. fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits
14.6 mag. fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 11.7 (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.eh2a5fvnJh (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-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.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_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.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-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.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-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits' -> 'wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits
WCS_IMAGE_NAME=wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits
WCS-calibrated image found: wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits
Checking if the catalog wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits.cat corresponding to the image wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits alredy exist and is non-empty...
Catalog wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits.cat corresponding to the image wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits
WCS catalog name: wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1510, passed=16419
Got 16419 stars (including 14877 good ones) from the SExtractor catalog wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits.cat
util/solve_plate_with_UCAC5 got 16419 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 949 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 949 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: 0.42"
Excluding outliers - 949 stars left (next iteration limit 1043)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits -region wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.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.PsWMIPd9lf (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-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.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_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.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-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.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-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits' -> 'wcs_Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits
WCS_IMAGE_NAME=wcs_Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits
WCS-calibrated image found: wcs_Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits
Checking if the catalog wcs_Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits.cat corresponding to the image wcs_Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits alredy exist and is non-empty...
Catalog wcs_Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits.cat corresponding to the image wcs_Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits
WCS catalog name: wcs_Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1544, passed=16335
Got 16335 stars (including 14759 good ones) from the SExtractor catalog wcs_Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits.cat
util/solve_plate_with_UCAC5 got 16335 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 953 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: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
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 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.42"
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 953 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits -region wcs_Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.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.GwKSwZhQjD (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_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.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_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits
WCS_IMAGE_NAME=wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits
WCS-calibrated image found: wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits
Checking if the catalog wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits.cat corresponding to the image wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits.cat corresponding to the image wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits
WCS catalog name: wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=640, passed=8478
Got 8478 stars (including 7832 good ones) from the SExtractor catalog wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits.cat
util/solve_plate_with_UCAC5 got 8478 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.56"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.56"
Estimated accuracy of the plate solution: 0.59"
Excluding outliers - 950 stars left (next iteration limit 1045)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits -region wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.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.pp4TqXYaQN (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_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.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_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits
WCS_IMAGE_NAME=wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits
WCS-calibrated image found: wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits
Checking if the catalog wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits.cat corresponding to the image wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits.cat corresponding to the image wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits
WCS catalog name: wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=640, passed=8361
Got 8361 stars (including 7715 good ones) from the SExtractor catalog wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits.cat
util/solve_plate_with_UCAC5 got 8361 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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 951 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: 0.58"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.57"
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 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.57"
Estimated accuracy of the plate solution: 0.60"
Excluding outliers - 950 stars left (next iteration limit 1045)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits -region wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.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-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits'
Saving fully-calibrated image wcs_Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/wcs_Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits'
Saving fully-calibrated image wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits'
Saving fully-calibrated image wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits'
Preparing the HTML report for the field Aur-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06267_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 06267_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:10:32.25 +32:10:42.9 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-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits
SExtractor catalog cache: saved Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits.cat to cache
SExtractor catalog cache: saved Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.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-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits
Creating symlink local_wcs_cache/wcs_Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.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-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits exists and is non-empty
wcs_Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits exists and is non-empty
wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits exists and is non-empty
wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 05:00:00.928 +29:59:47.56
Second-epoch image center 04:59:55.393 +29:56:10.02
Angular distance between the image centers 0.06 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:00:00.928 +29:59:47.56
Second-epoch image center 04:59:54.300 +29:56:16.19
Angular distance between the image centers 0.06 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 04:59:55.393 +29:56:10.02
Second-epoch second image center 04:59:54.300 +29:56:16.19
Angular distance between the image centers 0.00430 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-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits &> /tmp/tmp.eouKc1b1yI
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits &> /tmp/tmp.YXPAkExqFe
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits &> /tmp/tmp.CTR7P3d849
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits &> /tmp/tmp.jclUtVAXI2
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.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-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits and wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.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-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits and wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits.cat
Found non-empty wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits and wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits.cat
The reference image (wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits) and catalog (wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits.cat) found
'wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.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 6876 out of 137583 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.825942
a=0.000000 b=1.000000 c=22.825942
From vast_summary.log: estimated ref. image limiting mag.: -7.19
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.64
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.64
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 75 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.7 pix Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits
1.7 pix Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits
2.1 pix fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits
2.1 pix fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits
Limiting magnitude estimates:
15.6 mag. Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits
15.6 mag. Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits
14.7 mag. fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits
14.7 mag. fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 14.2 (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.eouKc1b1yI (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-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.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_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.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-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.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-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits' -> 'wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits
WCS_IMAGE_NAME=wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits
WCS-calibrated image found: wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits
Checking if the catalog wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits.cat corresponding to the image wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits alredy exist and is non-empty...
Catalog wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits.cat corresponding to the image wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits
WCS catalog name: wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=24, blended=14362, passed=137559
Got 137559 stars (including 122963 good ones) from the SExtractor catalog wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits.cat
util/solve_plate_with_UCAC5 got 137559 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 952 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 952 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: 0.41"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits -region wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.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.YXPAkExqFe (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-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.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_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.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-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.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-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits' -> 'wcs_Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits
WCS_IMAGE_NAME=wcs_Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits
WCS-calibrated image found: wcs_Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits
Checking if the catalog wcs_Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits.cat corresponding to the image wcs_Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits alredy exist and is non-empty...
Catalog wcs_Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits.cat corresponding to the image wcs_Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits
WCS catalog name: wcs_Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=26, blended=14447, passed=138047
Got 138047 stars (including 123396 good ones) from the SExtractor catalog wcs_Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits.cat
util/solve_plate_with_UCAC5 got 138047 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 953 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: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.43"
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 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.43"
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 953 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits -region wcs_Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.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.CTR7P3d849 (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_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.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_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits
WCS_IMAGE_NAME=wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits
WCS-calibrated image found: wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits
Checking if the catalog wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits.cat corresponding to the image wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits.cat corresponding to the image wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits
WCS catalog name: wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=25, blended=4538, passed=69903
Got 69903 stars (including 65250 good ones) from the SExtractor catalog wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits.cat
util/solve_plate_with_UCAC5 got 69903 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.57"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.54"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.54"
Estimated accuracy of the plate solution: 0.56"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits -region wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.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.jclUtVAXI2 (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_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.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_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits
WCS_IMAGE_NAME=wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits
WCS-calibrated image found: wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits
Checking if the catalog wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits.cat corresponding to the image wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits.cat corresponding to the image wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits
WCS catalog name: wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=4542, passed=70447
Got 70447 stars (including 65793 good ones) from the SExtractor catalog wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits.cat
util/solve_plate_with_UCAC5 got 70447 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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 954 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: 0.61"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.57"
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 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.57"
Estimated accuracy of the plate solution: 0.60"
Excluding outliers - 953 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits -region wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.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-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.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_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20.00sec_-15.00C_LIGHT_0031.fits
Saving fully-calibrated image wcs_Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.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_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/wcs_Aur-05-Q2b1x1_2026-02-11_20-26-33_20.00sec_-14.90C_LIGHT_0032.fits
Saving fully-calibrated image wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.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_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-30-21_20.00sec_-10.00C_LIGHT_0030.fits
Saving fully-calibrated image wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.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_2026-03-28_CI_Aur-05-Q2b1x1_213334_TTUQ2b1x1_24857_GkFmWbsz/wcs_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031.fits
Preparing the HTML report for the field Aur-05-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out159850.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159857.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159862.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159867.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159870.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159874.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159875.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159883.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159885.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159892.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159895.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159916.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159920.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160078.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160101.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160109.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160115.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160132.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160140.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160149.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160160.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160208.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20547.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out159976.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out160118.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out160210.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out63180.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 8s
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 159850_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 159850_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 04:51:07.27 +29:33:09.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 1.001 155337254722359296 072.78060669012 +29.55261958364 14.2865 13.5759 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.001#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 159857_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 159857_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:01:54.45 +30:27:41.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.55, MAG_FAINT_SEARCH_LIMIT=15.53)GAIADR2_OUTPUT=# 0.932 157138082970773504 075.47694768070 +30.46186221987 14.6774 13.7893 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.932#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 159862_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 159862_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 04:54:47.43 +30:17:18.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.13, MAG_FAINT_SEARCH_LIMIT=15.11)GAIADR2_OUTPUT=# 0.555 156905776779006080 073.69777011906 +30.28838225567 14.5935 13.9735 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.555#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 159867_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 159867_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:16:47.83 +31:09:30.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.11, MAG_FAINT_SEARCH_LIMIT=15.09)GAIADR2_OUTPUT=# 0.625 180357397728984064 079.19949394045 +31.15856907141 14.1686 13.5923 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.625#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 159870_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 159870_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 04:52:25.01 +29:02:17.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.99, MAG_FAINT_SEARCH_LIMIT=14.97)GAIADR2_OUTPUT=# 1.508 155261079182477312 073.10463157925 +29.03850170695 13.8057 13.0461 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.508#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 159871_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 159871_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 04:43:50.77 +28:01:39.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 159874_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 159874_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:18:31.32 +29:22:50.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 1.908 3446474688242818816 079.63089653740 +29.38018152810 13.7927 13.1795 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.908#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 159875_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 159875_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 04:35:50.80 +28:31:04.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 1.153 151994876812620544 068.96154467708 +28.51832962675 13.7191 12.8459 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.153#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 159876_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 159876_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 04:38:00.72 +29:52:18.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 159883_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 159883_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:22:59.27 +29:19:13.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 1.656 3446427138661843968 080.74691005731 +29.31990309979 13.9154 13.2682 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.656#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 159885_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 159885_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:20:40.34 +28:23:45.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)
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Considering the candidate 159892_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 159892_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 04:57:54.32 +28:06:32.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)
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Considering the candidate 159895_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 159895_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 04:52:12.10 +30:25:32.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 0.989 159905618160262656 073.05073396612 +30.42580254073 13.7365 13.0775 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.989#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 159902_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 159902_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 04:36:56.54 +28:25:19.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 159914_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 159914_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:14:52.03 +31:06:34.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 159916_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 159916_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 04:39:31.15 +27:42:58.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.17, MAG_FAINT_SEARCH_LIMIT=14.15)GAIADR2_OUTPUT=# 0.604 157700788108417664 069.87983812597 +27.71644051877 12.9256 12.1954 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.604#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 159917_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 159917_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:30:45.44 +28:44:37.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 159920_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 159920_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 04:46:16.20 +33:56:21.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 0.821 161556470446400256 071.56745062567 +33.93916441036 13.0131 12.3423 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.821#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 159923_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 159923_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 04:53:03.61 +26:37:35.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 159974_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 159974_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
Rejecting candidate due to large distance (15.6") between the two second-epoch detections
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Considering the candidate 159976_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
Preparing report for the candidate 159976_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
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Considering the candidate 159982_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 159982_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:26:32.95 +28:37:18.8 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 159986_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 159986_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 04:38:26.84 +26:55:00.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 159991_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 159991_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 04:51:21.93 +28:31:16.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 159997_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 159997_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
Rejecting candidate due to large distance (15.3") between the two second-epoch detections
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Considering the candidate 160006_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 160006_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 04:59:17.52 +32:33:38.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 160011_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 160011_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:24:45.00 +31:09:02.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 160013_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 160013_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:17:19.48 +33:12:06.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 160014_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 160014_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:18:28.42 +33:11:29.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 160016_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 160016_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 160026_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 160026_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:17:17.92 +33:11:43.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 160030_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 160030_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 04:48:18.81 +29:47:15.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 160034_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 160034_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 04:48:17.62 +29:45:38.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 160035_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 160035_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:26:49.17 +33:17:08.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 160037_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 160037_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
Rejecting candidate due to large distance (16.3") between the two second-epoch detections
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Considering the candidate 160038_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 160038_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:19:18.17 +33:59:46.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 160047_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 160047_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 04:39:20.36 +31:44:38.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 160055_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 160055_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:18:08.94 +33:24:15.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 160060_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 160060_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:29:46.98 +29:10:27.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 160062_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 160062_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:10:31.66 +30:49:30.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 160066_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 160066_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:19:34.72 +33:55:45.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 160070_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 160070_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:10:41.81 +30:48:34.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 160075_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 160075_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:15:58.52 +32:57:23.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 160076_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 160076_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:18:19.99 +33:23:32.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 160078_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 160078_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:21:08.06 +32:35:11.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 2.392 180841629521370880 080.28294911546 +32.58602194019 13.7077 12.7724 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.392#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 160080_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 160080_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:11:29.00 +29:54:24.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 160087_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 160087_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:10:59.67 +32:25:03.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 160097_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 160097_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 04:59:24.10 +31:04:55.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 160101_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 160101_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:30:08.76 +33:20:03.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 4.726 3449129287271043456 082.53676421105 +33.33292800019 14.0659 13.5824 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.726#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 160109_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 160109_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:31:51.72 +30:56:41.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 4.032 3446351542939548032 082.96530055938 +30.94605123489 13.8489 12.9502 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.032#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 160110_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 160110_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:15:53.05 +30:28:34.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 160115_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 160115_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 04:50:52.60 +29:08:41.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)GAIADR2_OUTPUT=# 0.805 155309079737025024 072.71912535100 +29.14502625821 13.9924 13.2246 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.805#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 160118_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
Preparing report for the candidate 160118_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
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Considering the candidate 160121_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 160121_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:05:57.91 +34:00:36.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 160122_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 160122_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:04:21.58 +28:40:48.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 160127_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 160127_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:27:07.14 +31:46:49.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 160128_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 160128_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 04:33:26.90 +30:56:08.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 160132_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 160132_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:12:52.11 +31:01:06.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 1.758 180436390766132096 078.21760569995 +31.01884578365 14.0429 13.3674 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.758#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 160134_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 160134_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 04:43:27.46 +32:27:49.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 160140_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 160140_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 04:57:11.74 +34:12:28.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 1.447 161756375404501376 074.29932863736 +34.20775873345 14.1605 13.3187 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.447#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 160149_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 160149_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:00:03.03 +30:01:06.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)GAIADR2_OUTPUT=# 1.360 156725349496991104 075.01300826166 +30.01834708003 14.6660 13.4161 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.360#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 160160_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 160160_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:02:01.16 +28:18:09.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.12, MAG_FAINT_SEARCH_LIMIT=15.10)GAIADR2_OUTPUT=# 3.412 155668310801710080 075.50563124877 +28.30313618245 14.2314 13.6351 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.412#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 160172_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 160172_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
Rejecting candidate due to large distance (16.4") between the two second-epoch detections
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Considering the candidate 160181_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 160181_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 160185_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 160185_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:09:50.96 +32:54:08.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 160192_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 160192_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
Rejecting candidate due to large distance (15.7") between the two second-epoch detections
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Considering the candidate 160197_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 160197_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
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Considering the candidate 160208_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 160208_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 04:47:03.14 +29:38:13.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 1.934 158308891054774144 071.76368012143 +29.63680421228 14.2528 13.4459 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.934#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 160210_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
Preparing report for the candidate 160210_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
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Considering the candidate 26468_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 26468_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
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Considering the candidate 33755_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 33755_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:22:00.54 +32:53:52.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 63180_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
Preparing report for the candidate 63180_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
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Considering the candidate 61547_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 61547_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 04:38:19.72 +31:18:46.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 47553_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 47553_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks
**** FOUND 05:10:32.21 +32:10:42.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20547_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031
The candidate 20547_fd_Aur-05-Q2b1x1_2026-03-28_21-31-06_20.00sec_-10.00C_LIGHT_0031 did not pass the final checks