This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 27.1058* 05 11 58.00 +25 53 11.3 12.3 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,2461126.6057,12.34,0.05,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 20260327.1057 12.34CV 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_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:11:58.00 +25:53:11.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-05-Q2b1x1_2026-02-11_20-25-42_20_00sec_-15_00C_LIGHT_0031_fits__*pix.png resample_wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20_00sec_-10_00C_LIGHT_0037_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_2026-03-26_21-31-42_20_00sec_-10_00C_LIGHT_0036_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_2026-03-26_21-32-31_20_00sec_-10_00C_LIGHT_0037_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_2026-03-26_21-31-42_20_00sec_-10_00C_LIGHT_0036_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,2461126.6057,13.07,0.05,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 20260327.1057 13.07CV 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_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:27:09.40 +30:55:44.8 ;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_2026-03-26_21-32-31_20_00sec_-10_00C_LIGHT_0037_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_2026-03-26_21-31-42_20_00sec_-10_00C_LIGHT_0036_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_2026-03-26_21-32-31_20_00sec_-10_00C_LIGHT_0037_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_2026-03-26_21-31-42_20_00sec_-10_00C_LIGHT_0036_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: 2461126.60603240 27.03.2026 02:32:31.199 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 6
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: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 13285
Objects passed selection criteria: 13252
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: 10888
Average stars matched: 10622.5 (97.5615 %)
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 Thu Mar 26 21:36:54 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: 2461126.60603240 27.03.2026 02:32:31.199 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 72
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: 92 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): 113159
Objects passed selection criteria: 112906
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 92146.2
Average stars matched: 88802.5 (96.3713 %)
Memory usage VmPeak: 2014560 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 26 21:40:06 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_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.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_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461126.60546542
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Plate-solving the images
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
wcs_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_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits exists and is non-empty
Saving wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits to local_wcs_cache/
'wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits' -> 'local_wcs_cache/wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits'
wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits exists and is non-empty
Saving wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits to local_wcs_cache/
'wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits' -> 'local_wcs_cache/wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.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 04:59:59.835 +30:00:19.72
Angular distance between the image centers 0.01 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:00:00.928 +29:59:47.56
Second-epoch image center 04:59:56.769 +30:00:26.72
Angular distance between the image centers 0.02 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 04:59:59.835 +30:00:19.72
Second-epoch second image center 04:59:56.769 +30:00:26.72
Angular distance between the image centers 0.01123 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.l1Kz0bcyzC
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.RFGmJI2AUc
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_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits &> /tmp/tmp.oGCUpAHUT3
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits &> /tmp/tmp.2DbebzENQX
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.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 2 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_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits
2.4 pix fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.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
14.5 mag. fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits
14.5 mag. fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits
All-image limiting magnitude estimate: 14.5 (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.l1Kz0bcyzC (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_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/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.RFGmJI2AUc (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_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/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.oGCUpAHUT3 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits
WCS_IMAGE_NAME=wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits
WCS-calibrated image found: wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits
Checking if the catalog wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits.cat corresponding to the image wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits.cat corresponding to the image wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.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_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits
WCS catalog name: wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=560, passed=8477
Got 8477 stars (including 7908 good ones) from the SExtractor catalog wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits.cat
util/solve_plate_with_UCAC5 got 8477 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (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 950 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.53"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.53"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 950 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: 0.55"
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_fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits -region wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.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.2DbebzENQX (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits
WCS_IMAGE_NAME=wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits
WCS-calibrated image found: wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits
Checking if the catalog wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits.cat corresponding to the image wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits.cat corresponding to the image wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.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_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits
WCS catalog name: wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=572, passed=8421
Got 8421 stars (including 7839 good ones) from the SExtractor catalog wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits.cat
util/solve_plate_with_UCAC5 got 8421 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (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: 0.55"
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_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits -region wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.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_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/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_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/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_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits'
Saving fully-calibrated image wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.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: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06267_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 06267_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks
**** FOUND 05:10:32.22 +32:10:42.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08628_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 08628_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks
**** FOUND 04:49:21.33 +30:55:35.4 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field 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_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.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_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.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_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.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_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits exists and is non-empty
wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.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 04:59:59.835 +30:00:19.72
Angular distance between the image centers 0.01 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 05:00:00.928 +29:59:47.56
Second-epoch image center 04:59:56.769 +30:00:26.72
Angular distance between the image centers 0.02 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 04:59:59.835 +30:00:19.72
Second-epoch second image center 04:59:56.769 +30:00:26.72
Angular distance between the image centers 0.01123 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.8Oyz337QXt
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.UpCezyVkBY
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_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits &> /tmp/tmp.GbBk0rwHcF
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits &> /tmp/tmp.BAD2Hf0s6A
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.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 54 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
2.3 pix fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits
2.2 pix fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.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
14.6 mag. fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits
14.6 mag. fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 14.1 (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.8Oyz337QXt (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_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/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.UpCezyVkBY (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_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/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.GbBk0rwHcF (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits
WCS_IMAGE_NAME=wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits
WCS-calibrated image found: wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits
Checking if the catalog wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits.cat corresponding to the image wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits.cat corresponding to the image wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.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_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits
WCS catalog name: wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=4357, passed=64761
Got 64761 stars (including 60306 good ones) from the SExtractor catalog wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits.cat
util/solve_plate_with_UCAC5 got 64761 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (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: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.52"
Estimated accuracy of the plate solution: 0.54"
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_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits -region wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.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.BAD2Hf0s6A (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits
WCS_IMAGE_NAME=wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits
WCS-calibrated image found: wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits
Checking if the catalog wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits.cat corresponding to the image wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits.cat corresponding to the image wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.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_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits
WCS catalog name: wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=4316, passed=65033
Got 65033 stars (including 60628 good ones) from the SExtractor catalog wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits.cat
util/solve_plate_with_UCAC5 got 65033 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.2'
Seting catalog search parameters based on the expected field of view 937.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013017 (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 0.010413 (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 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: 0.56"
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 953 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: 0.55"
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_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits -region wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.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_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/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_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/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_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-31-42_20.00sec_-10.00C_LIGHT_0036.fits
Saving fully-calibrated image wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-26_CI_Aur-05-Q2b1x1_213438_TTUQ2b1x1_21030_Sxsg8uh5/wcs_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037.fits
Preparing the HTML report for the field Aur-05-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out159849.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159850.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159863.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159865.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159866.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159874.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159885.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159888.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159901.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159903.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out159980.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160010.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160023.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160044.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160048.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160074.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160090.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160100.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160156.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160180.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160185.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160198.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160236.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160237.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160298.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160426.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160533.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out160616.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out159950.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out160013.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 7s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159849_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 159849_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks
**** FOUND 04:56:37.91 +32:30:00.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.40, MAG_FAINT_SEARCH_LIMIT=15.38)GAIADR2_OUTPUT=# 0.632 160757774031557760 074.15786996956 +32.50003554464 13.3910 12.1857 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.632#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159850_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 159850_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks
**** FOUND 05:08:10.41 +25:50:45.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.37, MAG_FAINT_SEARCH_LIMIT=15.35)GAIADR2_OUTPUT=# 1.627 3420104074377171328 077.04345263028 +25.84644640607 14.0960 13.3748 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.627#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159863_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 159863_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks
**** FOUND 05:01:59.94 +34:14:50.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 0.345 184985688845153664 075.49977224708 +34.24737810838 13.9685 13.4079 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.345#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159865_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 159865_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks
**** FOUND 04:43:50.77 +28:01:37.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 2.147 157767931334150144 070.96217532556 +28.02737346379 13.8340 13.0011 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.147#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159866_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 159866_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks
**** FOUND 05:02:17.64 +26:48:51.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159874_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 159874_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks
**** FOUND 05:30:26.35 +30:15:01.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 1.282 3446166829283134592 082.61019662574 +30.25056613644 13.5357 12.9273 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.282#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159877_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 159877_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks
**** FOUND 05:18:32.15 +29:23:05.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159885_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 159885_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks
**** FOUND 05:26:31.12 +31:54:07.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)GAIADR2_OUTPUT=# 1.292 3447394605816091264 081.63005008667 +31.90182093004 13.5879 12.9909 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.292#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159888_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 159888_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks
**** FOUND 05:21:25.83 +32:59:06.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 0.652 180950309374448896 080.35740972866 +32.98518076186 13.8071 13.3875 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.652#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159901_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 159901_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks
**** FOUND 05:14:51.96 +31:06:33.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159903_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 159903_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks
**** FOUND 04:53:03.70 +26:37:35.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 0.678 153602770833299584 073.26521417129 +26.62655160820 12.1887 11.1740 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.678#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159938_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 159938_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks
**** FOUND 05:22:15.66 +26:10:51.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159946_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 159946_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks
**** FOUND 05:15:29.67 +32:42:36.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159950_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
Preparing report for the candidate 159950_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159961_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 159961_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks
**** FOUND 05:26:32.94 +28:37:18.9 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159980_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 159980_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks
**** FOUND 04:51:21.95 +28:31:15.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 2.418 155132122787487872 072.84160076644 +28.52152096912 12.6812 11.9748 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.418#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159981_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 159981_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks
**** FOUND 04:38:26.86 +26:55:00.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159983_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 159983_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks
**** FOUND 05:28:55.16 +32:26:10.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159987_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 159987_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks
**** FOUND 04:59:17.62 +32:33:37.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 159998_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 159998_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks
**** FOUND 05:24:45.14 +31:09:02.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160005_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 160005_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks
**** FOUND 05:18:28.43 +33:11:29.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160010_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 160010_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks
**** FOUND 05:26:45.62 +30:29:13.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 2.221 3446971706156011264 081.69054938807 +30.48749604207 12.9674 12.3386 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.221#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160013_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
Preparing report for the candidate 160013_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160023_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 160023_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks
**** FOUND 05:17:19.51 +33:12:05.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 4.781 181115747215350016 079.33034975810 +33.20265211587 13.3222 12.7397 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.781#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160044_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 160044_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks
**** FOUND 05:17:17.90 +33:11:43.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.37, MAG_FAINT_SEARCH_LIMIT=14.35)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160048_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 160048_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks
**** FOUND 04:48:18.81 +29:47:15.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 0.461 158401902866571264 072.07844184694 +29.78766965032 13.0647 12.2921 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.461#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160056_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 160056_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks
**** FOUND 05:19:18.27 +33:59:46.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160059_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 160059_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks
**** FOUND 05:24:44.28 +31:08:25.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160067_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 160067_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks
**** FOUND 04:39:20.27 +31:44:38.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160074_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 160074_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks
**** FOUND 05:10:31.69 +30:49:30.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.50, MAG_FAINT_SEARCH_LIMIT=14.48)GAIADR2_OUTPUT=# 1.054 156425560781628928 077.63211988348 +30.82531270274 13.4967 12.9714 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.054#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160080_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 160080_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks
**** FOUND 05:29:47.00 +29:10:29.0 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160085_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 160085_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks
**** FOUND 04:48:17.63 +29:45:38.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160090_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 160090_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks
**** FOUND 05:18:19.94 +33:23:31.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 2.167 181218207955174784 079.58374215161 +33.39229988018 13.2589 12.1487 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.167#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160100_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 160100_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks
**** FOUND 05:10:41.72 +30:48:33.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 2.525 156422846362375296 077.67444411638 +30.80988224670 13.6874 13.0052 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.525#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160105_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 160105_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks
**** FOUND 05:19:34.67 +33:55:45.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160124_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 160124_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks
**** FOUND 05:28:57.19 +32:25:33.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160156_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 160156_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks
**** FOUND 05:15:53.00 +30:28:34.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)GAIADR2_OUTPUT=# 2.310 180183915409609984 078.97146830084 +30.47583178136 13.8443 13.2675 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.310#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160173_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 160173_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks
**** FOUND 04:59:24.09 +31:04:54.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160180_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 160180_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks
**** FOUND 04:59:38.16 +31:15:22.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 0.909 157421649593924224 074.90913733471 +31.25594305301 13.7089 12.9148 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.909#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160185_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 160185_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks
**** FOUND 05:11:29.03 +29:54:22.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 4.123 156157559117783168 077.86976660271 +29.90674457336 13.7937 13.0964 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.123#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160198_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 160198_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks
**** FOUND 05:04:39.06 +32:11:19.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 1.918 157545589467933696 076.16212452306 +32.18871776003 13.9014 13.2231 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.918#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160236_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 160236_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks
**** FOUND 04:52:36.06 +32:21:38.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 5.488 160413081432487808 073.15188696863 +32.36133602359 13.8886 12.9438 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.488#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160237_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 160237_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks
**** FOUND 05:10:59.74 +32:25:02.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 1.895 181433750891558144 077.74883314286 +32.41785505810 13.5478 12.5153 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.895#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160298_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 160298_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks
**** FOUND 04:58:15.24 +30:17:02.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.87, MAG_FAINT_SEARCH_LIMIT=14.85)GAIADR2_OUTPUT=# 0.976 156929927378514816 074.56340369869 +30.28425792805 13.9772 13.2609 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.976#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160304_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 160304_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks
**** FOUND 05:28:41.28 +33:56:25.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160426_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 160426_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks
**** FOUND 05:03:42.42 +33:35:52.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 3.856 184754413446459648 075.92659252847 +33.59909076544 13.7046 12.7113 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.856#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160431_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 160431_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks
**** FOUND 04:47:17.36 +33:06:51.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160491_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 160491_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks
**** FOUND 04:33:27.06 +30:56:06.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160533_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 160533_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks
**** FOUND 04:54:49.13 +33:30:55.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.26, MAG_FAINT_SEARCH_LIMIT=15.24)GAIADR2_OUTPUT=# 1.609 161614126087905024 073.70524293795 +33.51535626109 14.4643 13.7611 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.609#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160616_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 160616_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks
**** FOUND 05:13:59.40 +28:14:32.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.64, MAG_FAINT_SEARCH_LIMIT=15.62)GAIADR2_OUTPUT=# 0.375 3422300520652197504 078.49753319221 +28.24231665295 14.2974 13.5669 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.375#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 160621_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 160621_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks
**** FOUND 05:04:32.15 +26:05:15.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 67575_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 67575_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks
**** FOUND 04:49:21.34 +30:55:35.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 47553_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 47553_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks
**** FOUND 05:10:32.23 +32:10:42.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 61547_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037
The candidate 61547_fd_Aur-05-Q2b1x1_2026-03-26_21-32-31_20.00sec_-10.00C_LIGHT_0037 did not pass the final checks