This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 03 30.1240 2461129.6240 13.04 05:57:28.72 +38:36:59.4
172.88678 7.02877 galactic Aur Second-epoch detections are separated by 2.3" and 0.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J089.3707+38.6149 | 05:57:28.72 +38:36:59.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
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
ATO J089.3707+38.6149,2461129.6240,13.04,0.05,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
ATO J089.3707+38.6149 20260330.1240 13.04CV 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-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:57:28.72 +38:36:59.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png resample_wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20_00sec_-10_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png resample_wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20_00sec_-10_00C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png resample_wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20_00sec_-10_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png resample_wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20_00sec_-10_00C_LIGHT_0076_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.1240 2461129.6240 13.05 05:22:18.59 +36:11:57.2
171.23848 -0.17259 galactic Aur Second-epoch detections are separated by 4.0" and 1.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:22:18.59 +36:11:57.2 (user input) | T | P | (position from user input) SpType: A0III (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461129.6240,13.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260330.1240 13.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:22:18.59 +36:11:57.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png resample_wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20_00sec_-10_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png resample_wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20_00sec_-10_00C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png resample_wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20_00sec_-10_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png resample_wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20_00sec_-10_00C_LIGHT_0076_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461129.6240,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260330.1240 13.30CV 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-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:42:34.68 +37:09:44.8 ;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-03-Q2b1x1_2026-02-11_20-51-30_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png resample_wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20_00sec_-10_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png resample_wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20_00sec_-10_00C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png resample_wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20_00sec_-10_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png resample_wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20_00sec_-10_00C_LIGHT_0076_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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
ASASSN-V J050056.14+380913.4,2461129.6240,11.04,0.05,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
ASASSN-V J050056.14+380913.4 20260330.1240 11.04CV 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-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:00:56.62 +38:09:15.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png resample_wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20_00sec_-10_00C_LIGHT_0077_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png resample_wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20_00sec_-10_00C_LIGHT_0076_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png resample_wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20_00sec_-10_00C_LIGHT_0077_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20_00sec_-14_90C_LIGHT_0053_fits__*pix.png resample_wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20_00sec_-10_00C_LIGHT_0076_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461083.61922233 12.02.2026 02:51:30.809 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
First image: 2461083.61922233 12.02.2026 02:51:30.809 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
Last image: 2461129.62420463 30.03.2026 02:58:41.280 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.58
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 6 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 23942
Objects passed selection criteria: 23815
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 17264.2
Average stars matched: 16756.5 (97.059 %)
Memory usage VmPeak: 129656 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Mar 29 22:11:03 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: 2461083.61922233 12.02.2026 02:51:30.809 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
First image: 2461083.61922233 12.02.2026 02:51:30.809 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
Last image: 2461129.62420463 30.03.2026 02:58:41.280 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 132
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.24
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: 54 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): 185314
Objects passed selection criteria: 184860
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 136668
Average stars matched: 131735 (96.3909 %)
Memory usage VmPeak: 2016448 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Mar 29 22:16:40 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-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits
SExtractor catalog cache: saved Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits.cat to cache
SExtractor catalog cache: saved Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.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-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461129.62371900
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits exists and is non-empty
Saving wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits to local_wcs_cache/
'wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits' -> 'local_wcs_cache/wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits'
wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits exists and is non-empty
Saving wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits to local_wcs_cache/
'wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits' -> 'local_wcs_cache/wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits'
wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits exists and is non-empty
Saving wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits to local_wcs_cache/
'wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits' -> 'local_wcs_cache/wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits'
wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits exists and is non-empty
Saving wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits to local_wcs_cache/
'wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits' -> 'local_wcs_cache/wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits'
The image scale is 5.91"/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 05:27:33.978 +37:59:21.26
Second-epoch image center 05:27:16.736 +38:01:53.93
Angular distance between the image centers 0.07 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 05:27:33.978 +37:59:21.26
Second-epoch image center 05:27:16.996 +38:01:55.28
Angular distance between the image centers 0.07 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 05:27:16.736 +38:01:53.93
Second-epoch second image center 05:27:16.996 +38:01:55.28
Angular distance between the image centers 0.00093 deg.
###################################
ERROR: no shift applied between second-epoch images! The distance between image centers is 0.00093 deg. (min. required shift: 0.00164 deg.)
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits &> /tmp/tmp.YSSGe2iKRp
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits &> /tmp/tmp.0lgehz6FSc
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits &> /tmp/tmp.uDFBwkMWGj
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits &> /tmp/tmp.qzd5wg6UKX
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.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-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits and wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.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-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits and wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits.cat
Found non-empty wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits and wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits.cat
The reference image (wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits) and catalog (wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits.cat) found
'wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.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 6465 out of 30329 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.940226
a=0.000000 b=1.000000 c=22.940226
From vast_summary.log: estimated ref. image limiting mag.: -7.58
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.36
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.36
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
2.1 pix Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits
2.5 pix fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits
2.5 pix fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits
Limiting magnitude estimates:
15.4 mag. Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
15.4 mag. Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits
14.0 mag. fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits
14.0 mag. fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 11.2 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.YSSGe2iKRp (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-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.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-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.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-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits' -> 'wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
WCS_IMAGE_NAME=wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
WCS-calibrated image found: wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
Checking if the catalog wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits.cat corresponding to the image wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits alredy exist and is non-empty...
Catalog wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits.cat corresponding to the image wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
WCS catalog name: wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3460, passed=30329
Got 30329 stars (including 26832 good ones) from the SExtractor catalog wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits.cat
util/solve_plate_with_UCAC5 got 30329 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 943.3'
Seting catalog search parameters based on the expected field of view 943.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013101 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010481 (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 905 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 1.84"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 2.17"
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 920 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 2.14"
Estimated accuracy of the plate solution: 1.18"
Excluding outliers - 912 stars left (next iteration limit 985)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits -region wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.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.0lgehz6FSc (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-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.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-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.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-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits' -> 'wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits
WCS_IMAGE_NAME=wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits
WCS-calibrated image found: wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits
Checking if the catalog wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits.cat corresponding to the image wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits alredy exist and is non-empty...
Catalog wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits.cat corresponding to the image wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits
WCS catalog name: wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=3436, passed=30261
Got 30261 stars (including 26784 good ones) from the SExtractor catalog wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits.cat
util/solve_plate_with_UCAC5 got 30261 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 944 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: 0.52"
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 944 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: 0.48"
Excluding outliers - 943 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits -region wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.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.uDFBwkMWGj (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits
WCS_IMAGE_NAME=wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits
WCS-calibrated image found: wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits
Checking if the catalog wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits.cat corresponding to the image wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits.cat corresponding to the image wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits
WCS catalog name: wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=625, passed=9900
Got 9900 stars (including 9266 good ones) from the SExtractor catalog wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits.cat
util/solve_plate_with_UCAC5 got 9900 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.64"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.65"
Estimated accuracy of the plate solution: 0.73"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits -region wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.qzd5wg6UKX (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits
WCS_IMAGE_NAME=wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits
WCS-calibrated image found: wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits
Checking if the catalog wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits.cat corresponding to the image wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits.cat corresponding to the image wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits
WCS catalog name: wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=641, passed=9821
Got 9821 stars (including 9173 good ones) from the SExtractor catalog wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits.cat
util/solve_plate_with_UCAC5 got 9821 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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 948 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: 0.71"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.66"
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 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.67"
Estimated accuracy of the plate solution: 0.75"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits -region wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits'
Saving fully-calibrated image wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits'
Saving fully-calibrated image wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits'
Saving fully-calibrated image wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits'
Preparing the HTML report for the field Aur-03-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 51965_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 51965_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:26:54.61 +36:54:12.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 10199_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 10199_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 06:01:07.03 +39:40:14.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 07937_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 07937_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:54:39.24 +40:33:26.7 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-03-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-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits
SExtractor catalog cache: saved Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits.cat to cache
SExtractor catalog cache: saved Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.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-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
Creating symlink local_wcs_cache/wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits exists and is non-empty
wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits exists and is non-empty
wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits exists and is non-empty
wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits exists and is non-empty
The image scale is 5.91"/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 05:27:33.978 +37:59:21.26
Second-epoch image center 05:27:16.736 +38:01:53.93
Angular distance between the image centers 0.07 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 05:27:33.978 +37:59:21.26
Second-epoch image center 05:27:16.996 +38:01:55.28
Angular distance between the image centers 0.07 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 05:27:16.736 +38:01:53.93
Second-epoch second image center 05:27:16.996 +38:01:55.28
Angular distance between the image centers 0.00093 deg.
###################################
ERROR: no shift applied between second-epoch images! The distance between image centers is 0.00093 deg. (min. required shift: 0.00164 deg.)
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits &> /tmp/tmp.87y4SqjMmz
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits &> /tmp/tmp.LXP1YWzx3C
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits &> /tmp/tmp.tmkCRNS5If
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits &> /tmp/tmp.MWo0VBViXF
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.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-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits and wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.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-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits and wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits.cat
Found non-empty wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits and wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits.cat
The reference image (wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits) and catalog (wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits.cat) found
'wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.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 6645 out of 230190 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.800367
a=0.000000 b=1.000000 c=22.800367
From vast_summary.log: estimated ref. image limiting mag.: -7.24
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.56
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.56
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 105 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
1.9 pix Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits
2.3 pix fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits
2.3 pix fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits
Limiting magnitude estimates:
15.6 mag. Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
15.5 mag. Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits
14.0 mag. fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits
14.0 mag. fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 13.5 (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.87y4SqjMmz (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-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.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-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.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-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits' -> 'wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
WCS_IMAGE_NAME=wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
WCS-calibrated image found: wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
Checking if the catalog wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits.cat corresponding to the image wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits alredy exist and is non-empty...
Catalog wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits.cat corresponding to the image wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
WCS catalog name: wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=41, blended=35441, passed=230149
Got 230149 stars (including 194360 good ones) from the SExtractor catalog wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits.cat
util/solve_plate_with_UCAC5 got 230149 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 943.3'
Seting catalog search parameters based on the expected field of view 943.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013101 (47.2 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010481 (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 910 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: 2.04"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 2.04"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 924 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 2.03"
Estimated accuracy of the plate solution: 1.02"
Excluding outliers - 919 stars left (next iteration limit 990)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits -region wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.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.LXP1YWzx3C (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-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.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-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.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-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits' -> 'wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits
WCS_IMAGE_NAME=wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits
WCS-calibrated image found: wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits
Checking if the catalog wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits.cat corresponding to the image wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits alredy exist and is non-empty...
Catalog wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits.cat corresponding to the image wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits
WCS catalog name: wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=62, blended=35436, passed=229960
Got 229960 stars (including 194138 good ones) from the SExtractor catalog wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits.cat
util/solve_plate_with_UCAC5 got 229960 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 942 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: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.50"
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 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.50"
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 940 stars left (next iteration limit 1034)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits -region wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.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.tmkCRNS5If (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits
WCS_IMAGE_NAME=wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits
WCS-calibrated image found: wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits
Checking if the catalog wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits.cat corresponding to the image wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits.cat corresponding to the image wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits
WCS catalog name: wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=5626, passed=76291
Got 76291 stars (including 70559 good ones) from the SExtractor catalog wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits.cat
util/solve_plate_with_UCAC5 got 76291 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 947 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: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.61"
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 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.61"
Estimated accuracy of the plate solution: 0.67"
Excluding outliers - 943 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits -region wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.MWo0VBViXF (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits
WCS_IMAGE_NAME=wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits
WCS-calibrated image found: wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits
Checking if the catalog wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits.cat corresponding to the image wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits.cat corresponding to the image wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits
WCS catalog name: wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=5511, passed=76356
Got 76356 stars (including 70743 good ones) from the SExtractor catalog wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits.cat
util/solve_plate_with_UCAC5 got 76356 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (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 0.010412 (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 948 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: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.62"
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 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.62"
Estimated accuracy of the plate solution: 0.69"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits -region wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/wcs_Aur-03-Q2b1x1_2026-02-11_20-51-30_20.00sec_-14.90C_LIGHT_0053.fits
Saving fully-calibrated image wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/wcs_Aur-03-Q2b1x1_2026-02-11_20-52-13_20.00sec_-14.90C_LIGHT_0054.fits
Saving fully-calibrated image wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-57-59_20.00sec_-10.00C_LIGHT_0076.fits
Saving fully-calibrated image wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Aur-03-Q2b1x1_220504_TTUQ2b1x1_3216_iQDqkdbK/wcs_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077.fits
Preparing the HTML report for the field Aur-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out225631.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out258846.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out258848.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out258865.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out258866.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out258869.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out258873.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out259023.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out259065.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out259087.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out259091.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out259151.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out259204.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out259213.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out259244.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out259260.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out259267.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out259268.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out259274.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out259296.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out259303.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out259304.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out259308.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out259338.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out259368.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out259387.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out259424.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out259431.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out259438.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out259440.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out259456.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out259468.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out259473.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out259479.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out259500.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out259518.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out259537.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out259580.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out124480.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out259299.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out259343.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out259412.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 18s
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: 3s
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Considering the candidate 258832_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 258832_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 258842_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 258842_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:28:11.43 +35:31:10.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 258846_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 258846_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:39:30.29 +38:31:13.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 1.821 190075053294241536 084.87660972854 +38.52002020376 13.5149 12.9383 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.821#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 258848_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 258848_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:33:36.81 +35:02:12.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 1.186 183009278037441792 083.40363598799 +35.03649934629 13.0115 12.1716 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.186#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 258857_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 258857_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:28:56.32 +34:52:20.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 258864_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 258864_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.1 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 258865_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 258865_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:04:13.60 +35:30:05.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 2.810 185204800896636928 076.05714938858 +35.50071442944 13.2707 12.7609 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.810#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 258866_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 258866_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:21:20.80 +35:28:38.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.02, MAG_FAINT_SEARCH_LIMIT=14.00)GAIADR2_OUTPUT=# 2.948 183644731336288000 080.33747725292 +35.47776237729 13.1581 12.5895 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.948#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 258869_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 258869_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:29:33.82 +34:03:11.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 2.160 182565972993305472 082.39160269807 +34.05324801484 13.1568 12.7834 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.160#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 258873_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 258873_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:31:51.62 +36:03:45.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 0.794 183407339905581568 082.96532368863 +36.06264549300 12.5791 12.0832 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.794#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 258947_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 258947_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:19:15.46 +40:07:53.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 258995_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 258995_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:27:41.39 +34:26:43.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 259023_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259023_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:49:06.55 +39:13:07.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.00, MAG_FAINT_SEARCH_LIMIT=12.98)GAIADR2_OUTPUT=# 1.633 191431988081827712 087.27779159080 +39.21843049832 11.7217 10.9369 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.633#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 259033_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259033_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:59:31.33 +37:13:43.1 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 259047_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259047_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:24:47.20 +37:21:51.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 259055_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259055_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:10:27.38 +37:19:05.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 259065_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259065_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:36:18.61 +34:10:46.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 0.485 3449524561700715392 084.07737898627 +34.17943668612 12.2593 11.9864 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.485#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 259066_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259066_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 259087_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259087_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:27:40.68 +34:43:56.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.18, MAG_FAINT_SEARCH_LIMIT=13.16)GAIADR2_OUTPUT=# 1.455 182855037174064512 081.91984122513 +34.73204229306 12.0902 11.5747 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.455#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 259088_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259088_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:00:16.22 +39:38:31.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 259091_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259091_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:50:56.97 +37:20:27.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.42, MAG_FAINT_SEARCH_LIMIT=13.40)GAIADR2_OUTPUT=# 1.403 3456201827096096896 087.73750999629 +37.34051417104 12.1063 11.0900 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.403#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 259101_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259101_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 259103_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259103_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 259104_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259104_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 259128_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259128_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:19:01.48 +41:06:59.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259132_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259132_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:26:40.59 +34:23:17.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 259134_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259134_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:06:25.39 +34:49:30.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259144_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259144_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:45:51.08 +37:37:56.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259151_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259151_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:14:49.39 +39:31:05.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 2.500 188694887024070400 078.70528210737 +39.51751089000 11.4625 10.1709 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.500#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 259158_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259158_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:24:49.81 +37:22:49.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 259177_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259177_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:30:54.16 +39:49:18.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 259178_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259178_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:06:43.73 +41:15:38.8 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 259190_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259190_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:18:56.51 +41:04:18.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259201_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259201_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:17:19.55 +39:28:45.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259204_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259204_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 06:00:17.32 +34:30:12.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)GAIADR2_OUTPUT=# 3.575 3451875695515412224 090.07190042027 +34.50250380406 12.6710 11.7512 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.575#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 259210_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259210_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 259212_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259212_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 259213_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259213_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:29:49.45 +35:22:28.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.75, MAG_FAINT_SEARCH_LIMIT=13.73)GAIADR2_OUTPUT=# 1.523 183255847820054912 082.45652394749 +35.37439980675 12.7621 12.3777 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.523#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 259244_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259244_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:32:38.79 +39:32:33.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.83, MAG_FAINT_SEARCH_LIMIT=13.81)GAIADR2_OUTPUT=# 2.312 190759499281586176 083.16160242297 +39.54202476105 13.0936 12.7575 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.312#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 259251_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259251_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:13:19.33 +38:28:12.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 259260_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259260_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:19:59.36 +39:20:12.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 1.675 187964536428306048 079.99742402138 +39.33645681293 12.8694 12.4905 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.675#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 259264_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259264_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:59:59.25 +37:12:24.8 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 259265_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259265_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:27:57.01 +33:47:20.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259267_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259267_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:30:14.49 +40:29:50.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.93, MAG_FAINT_SEARCH_LIMIT=13.91)GAIADR2_OUTPUT=# 1.721 193864863715926784 082.56025127553 +40.49700354086 13.0273 12.7214 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.721#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 259268_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259268_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:52:30.93 +40:09:44.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 2.017 191598976410246400 088.12960797702 +40.16236073689 13.1196 12.5732 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.017#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 259274_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259274_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:06:33.76 +35:29:44.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.85, MAG_FAINT_SEARCH_LIMIT=13.83)GAIADR2_OUTPUT=# 2.520 185520566893531136 076.64129652703 +35.49513464354 13.0098 12.3434 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.520#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 259286_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259286_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:18:32.25 +40:27:42.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 259287_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259287_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:44:55.76 +38:31:30.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259296_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259296_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:49:38.79 +40:57:59.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)
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Considering the candidate 259299_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
Preparing report for the candidate 259299_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
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Considering the candidate 259300_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259300_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:27:40.99 +33:56:59.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259303_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259303_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:27:45.99 +34:44:28.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.01, MAG_FAINT_SEARCH_LIMIT=13.99)GAIADR2_OUTPUT=# 2.432 182855075830522368 081.94228195240 +34.74087161080 13.1674 12.7783 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.432#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 259304_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259304_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:38:11.86 +37:43:59.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 2.369 189602705672883584 084.54949039302 +37.73251114839 13.2937 12.8397 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.369#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 259308_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259308_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:14:24.32 +39:22:50.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.90, MAG_FAINT_SEARCH_LIMIT=13.88)GAIADR2_OUTPUT=# 0.855 188668430025536000 078.60163318875 +39.38069853517 12.9473 12.3469 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.855#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 259318_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259318_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:19:22.74 +40:08:57.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259323_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259323_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:09:36.28 +38:39:31.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259324_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259324_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:59:23.93 +40:02:38.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259325_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259325_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:17:57.89 +35:10:55.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259338_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259338_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:15:04.68 +35:21:47.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.00, MAG_FAINT_SEARCH_LIMIT=13.98)GAIADR2_OUTPUT=# 2.268 182387199271878144 078.77004046377 +35.36282773824 13.0420 12.4869 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.268#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 259343_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
Preparing report for the candidate 259343_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
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Considering the candidate 259361_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259361_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:20:49.14 +37:27:02.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259368_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259368_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:52:18.95 +38:34:07.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 2.157 3457973312125389056 088.07956881282 +38.56835981736 13.2635 12.6942 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.157#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 259387_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259387_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:25:33.37 +38:02:26.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 4.414 184594297066525312 081.38783294889 +38.03986598579 13.4523 12.6225 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.414#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 259406_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259406_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 259409_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259409_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 259410_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259410_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:45:59.70 +41:14:54.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259411_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259411_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:14:44.86 +39:31:20.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259412_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
Preparing report for the candidate 259412_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
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Considering the candidate 259421_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259421_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:13:26.29 +35:39:15.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259424_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259424_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:41:54.78 +34:03:57.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 2.205 3449373997326609920 085.47845349663 +34.06524435321 13.2442 12.7143 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.205#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 259431_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259431_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:39:22.18 +37:34:53.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 4.363 189421256192022656 084.84251180248 +37.58029053936 14.0015 13.2928 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.363#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 259435_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259435_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:07:48.50 +39:51:26.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259437_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259437_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:19:27.54 +34:00:25.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 259438_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259438_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:10:57.79 +39:16:01.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 5.111 188486392132059008 077.74250280054 +39.26654502221 13.3341 12.8014 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.111#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 259440_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259440_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:51:18.23 +35:41:00.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.36, MAG_FAINT_SEARCH_LIMIT=14.34)GAIADR2_OUTPUT=# 1.104 3455187531916399872 087.82633244314 +35.68348500956 13.6658 13.0253 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.104#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 259449_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259449_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:41:00.67 +39:37:07.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259456_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259456_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:13:34.44 +35:40:04.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 2.345 185395218270056576 078.39420385032 +35.66825618290 13.1112 12.2474 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.345#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 259466_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259466_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:32:56.12 +36:20:33.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259468_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259468_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:06:28.80 +35:34:53.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 0.431 185526236250336256 076.61992264119 +35.58149080035 13.0782 12.4248 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.431#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 259473_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259473_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:23:33.13 +34:41:39.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)GAIADR2_OUTPUT=# 3.335 182810133292244096 080.88865696234 +34.69350167388 13.6385 13.0871 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.335#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 259479_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259479_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:29:36.14 +35:06:45.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.15, MAG_FAINT_SEARCH_LIMIT=14.13)
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Considering the candidate 259488_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259488_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:30:42.92 +39:52:01.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259498_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259498_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:35:43.52 +38:03:13.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259500_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259500_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:36:04.05 +36:38:32.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 2.205 189254641523843456 084.01702345736 +36.64181579515 13.6792 13.2310 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.205#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 259503_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259503_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:13:15.88 +40:10:23.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259518_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259518_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:22:16.90 +37:03:23.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 3.280 184443767053322112 080.57154166276 +37.05671108799 13.3559 12.5507 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.280#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 259527_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259527_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:45:44.43 +40:28:53.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 259536_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259536_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.3 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 259537_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259537_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:29:39.66 +35:08:06.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 0.614 183243169076710656 082.41535439159 +35.13485242559 13.5163 12.8703 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.614#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 259555_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259555_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:24:37.15 +36:11:00.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259570_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259570_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:20:43.43 +37:24:54.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259580_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259580_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:21:23.41 +35:28:40.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 3.005 183644731336286592 080.34835739915 +35.47853302510 13.3701 12.8531 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.005#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 259585_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259585_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:33:44.07 +36:26:32.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259600_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259600_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:32:13.85 +34:57:20.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259633_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259633_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:08:39.82 +37:35:36.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 259639_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 259639_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.2 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 74075_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 74075_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 06:00:51.52 +39:44:39.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 124480_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
Preparing report for the candidate 124480_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
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Considering the candidate 225631_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 225631_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:07:03.58 +34:02:50.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)
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Considering the candidate 149080_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 149080_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:54:37.39 +36:34:06.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 57186_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 57186_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:54:39.17 +40:33:26.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 150552_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 150552_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:26:54.60 +36:54:12.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 102878_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 102878_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 05:20:15.00 +39:06:52.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 77572_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 77572_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks
**** FOUND 06:01:06.99 +39:40:14.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 164112_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077
The candidate 164112_fd_Aur-03-Q2b1x1_2026-03-29_21-58-41_20.00sec_-10.00C_LIGHT_0077 did not pass the final checks