This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp
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 30.4032 2461129.9032 10.55 20:19:43.31 +22:34:26.2
63.22264 -7.68663 galactic Vul Second-epoch detections are separated by 0.3" and 5.1 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 | Gaia DR3 1829526948510405504 | 20:19:41.68 +22:34:26.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.225+/-0.031 (F)
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
Gaia DR3 1829526948510405504,2461129.9032,10.55,0.05,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
Gaia DR3 1829526948510405504 20260330.4032 10.55CV 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/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:19:43.31 +22:34:26.2 ;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_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20_00sec_-10_00C_LIGHT_0342_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20_00sec_-10_00C_LIGHT_0341_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20_00sec_-10_00C_LIGHT_0342_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20_00sec_-10_00C_LIGHT_0341_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
Gaia DR2 1823078690777998592,2461129.9032,12.82,0.05,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
Gaia DR2 1823078690777998592 20260330.4032 12.82CV 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/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:00:56.83 +19:31:53.1 ;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_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20_00sec_-10_00C_LIGHT_0342_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20_00sec_-10_00C_LIGHT_0341_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20_00sec_-10_00C_LIGHT_0342_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20_00sec_-10_00C_LIGHT_0341_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461129.9032,12.93,0.05,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 20260330.4032 12.93CV 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/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:04:21.03 +22:35:15.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20_00sec_-10_00C_LIGHT_0342_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20_00sec_-10_00C_LIGHT_0341_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20_00sec_-10_00C_LIGHT_0342_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20_00sec_-10_00C_LIGHT_0341_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 30.4032* 20 32 24.70 +19 29 38.6 12.4 U Del 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J2032245+192934,2461129.9032,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J2032245+192934 20260330.4032 12.40CV 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/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 20:32:24.70 +19:29:38.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20_00sec_-10_00C_LIGHT_0342_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20_00sec_-10_00C_LIGHT_0341_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20_00sec_-10_00C_LIGHT_0342_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20_00sec_-10_00C_LIGHT_0341_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: 2461098.99517851 27.02.2026 11:52:53.423 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
First image: 2461098.99517851 27.02.2026 11:52:53.423 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
Last image: 2461129.90350668 30.03.2026 09:40:52.977 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.96
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 20447
Objects passed selection criteria: 20355
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: 14611
Average stars matched: 14212.8 (97.2743 %)
Memory usage VmPeak: 125880 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 Mon Mar 30 04:42:55 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: 2461098.99517851 27.02.2026 11:52:53.423 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
First image: 2461098.99517851 27.02.2026 11:52:53.423 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
Last image: 2461129.90350668 30.03.2026 09:40:52.977 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 124
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.61
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: 42 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): 194665
Objects passed selection criteria: 194162
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 147042
Average stars matched: 141657 (96.3376 %)
Memory usage VmPeak: 2022724 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 Mon Mar 30 04:47:45 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/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits
SExtractor catalog cache: saved Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat to cache
SExtractor catalog cache: saved Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.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/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.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: 2461129.90293443
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits exists and is non-empty
Saving wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits to local_wcs_cache/
'wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits' -> 'local_wcs_cache/wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits'
wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits exists and is non-empty
Saving wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits to local_wcs_cache/
'wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits' -> 'local_wcs_cache/wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits'
wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits exists and is non-empty
Saving wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits to local_wcs_cache/
'wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits' -> 'local_wcs_cache/wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits'
wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits exists and is non-empty
Saving wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits to local_wcs_cache/
'wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits' -> 'local_wcs_cache/wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 20:18:28.950 +22:00:14.29
Second-epoch image center 20:18:20.398 +22:03:41.94
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 20:18:28.950 +22:00:14.29
Second-epoch image center 20:18:18.230 +22:03:36.62
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 20:18:20.398 +22:03:41.94
Second-epoch second image center 20:18:18.230 +22:03:36.62
Angular distance between the image centers 0.00850 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/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits &> /tmp/tmp.NDkbR8Yvdk
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits &> /tmp/tmp.MZLj4iorDx
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits &> /tmp/tmp.qcZa4LQYDr
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits &> /tmp/tmp.pi5KiOFaZG
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits
Calibrating the magnitude scale
Found non-empty wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.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_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits and wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.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_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits and wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat
Found non-empty wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits and wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat
The reference image (wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits) and catalog (wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat) found
'wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.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 14549 out of 24638 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.758582
a=0.000000 b=1.000000 c=22.758582
From vast_summary.log: estimated ref. image limiting mag.: -7.96
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.80
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.80
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
2.0 pix Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
2.5 pix fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits
2.5 pix fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits
Limiting magnitude estimates:
14.8 mag. Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
14.8 mag. Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
13.5 mag. fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits
13.5 mag. fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits
All-image limiting magnitude estimate: 13.5 (SNR ) 10.8 (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.NDkbR8Yvdk (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/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.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_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits' -> 'wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
WCS_IMAGE_NAME=wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
WCS-calibrated image found: wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
Checking if the catalog wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat corresponding to the image wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits alredy exist and is non-empty...
Catalog wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat corresponding to the image wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
WCS catalog name: wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2463, passed=24638
Got 24638 stars (including 22152 good ones) from the SExtractor catalog wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat
util/solve_plate_with_UCAC5 got 24638 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (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 0.010470 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.68"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 935 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: 0.58"
Excluding outliers - 935 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits -region wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.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.MZLj4iorDx (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/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.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_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits' -> 'wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
WCS_IMAGE_NAME=wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
WCS-calibrated image found: wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
Checking if the catalog wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat corresponding to the image wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits alredy exist and is non-empty...
Catalog wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat corresponding to the image wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
WCS catalog name: wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2477, passed=24779
Got 24779 stars (including 22281 good ones) from the SExtractor catalog wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat
util/solve_plate_with_UCAC5 got 24779 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (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 0.010470 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.67"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.70"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.70"
Estimated accuracy of the plate solution: 0.56"
Excluding outliers - 936 stars left (next iteration limit 1029)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits -region wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.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.qcZa4LQYDr (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_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.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_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits
WCS_IMAGE_NAME=wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits
WCS-calibrated image found: wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits
Checking if the catalog wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits.cat corresponding to the image wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits.cat corresponding to the image wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits
WCS catalog name: wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=635, passed=8490
Got 8490 stars (including 7849 good ones) from the SExtractor catalog wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits.cat
util/solve_plate_with_UCAC5 got 8490 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.5'
Seting catalog search parameters based on the expected field of view 938.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013035 (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 0.010428 (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 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.61"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.58"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.59"
Estimated accuracy of the plate solution: 0.66"
Excluding outliers - 934 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits -region wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.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.pi5KiOFaZG (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_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.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_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits
WCS_IMAGE_NAME=wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits
WCS-calibrated image found: wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits
Checking if the catalog wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits.cat corresponding to the image wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits.cat corresponding to the image wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits
WCS catalog name: wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=658, passed=8744
Got 8744 stars (including 8079 good ones) from the SExtractor catalog wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits.cat
util/solve_plate_with_UCAC5 got 8744 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.4'
Seting catalog search parameters based on the expected field of view 938.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013033 (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 0.010427 (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 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.61"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.59"
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 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.59"
Estimated accuracy of the plate solution: 0.67"
Excluding outliers - 935 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits -region wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.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_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits'
Saving fully-calibrated image wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits'
Saving fully-calibrated image wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits'
Saving fully-calibrated image wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits'
Preparing the HTML report for the field Vul-02-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out14123.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 12s
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 31401_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 31401_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 19:51:30.77 +25:21:39.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 31513_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 31513_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 19:52:33.25 +19:06:23.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17681_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 17681_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 19:56:28.91 +23:54:46.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14123_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
Preparing report for the candidate 14123_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 13s
Prepared the HTML report for the field Vul-02-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 ####
20:19:43.31 +22:34:26.2
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/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits
SExtractor catalog cache: saved Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat to cache
SExtractor catalog cache: saved Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
Creating symlink local_wcs_cache/wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
Creating symlink local_wcs_cache/wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits
Creating symlink local_wcs_cache/wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.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_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits exists and is non-empty
wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits exists and is non-empty
wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits exists and is non-empty
wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 20:18:28.950 +22:00:14.29
Second-epoch image center 20:18:20.398 +22:03:41.94
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 20:18:28.950 +22:00:14.29
Second-epoch image center 20:18:18.230 +22:03:36.62
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 20:18:20.398 +22:03:41.94
Second-epoch second image center 20:18:18.230 +22:03:36.62
Angular distance between the image centers 0.00850 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/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits &> /tmp/tmp.2r9RGCfxZX
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits &> /tmp/tmp.s6KNMSFMGt
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits &> /tmp/tmp.0sUzmGmFco
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits &> /tmp/tmp.XQOdtfM6WV
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits
Calibrating the magnitude scale
Found non-empty wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.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_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits and wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.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_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits and wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat
Found non-empty wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits and wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat
The reference image (wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits) and catalog (wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat) found
'wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.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 17496 out of 232861 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.547121
a=0.000000 b=1.000000 c=22.547121
From vast_summary.log: estimated ref. image limiting mag.: -7.61
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.94
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.94
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 87 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.8 pix Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
1.9 pix Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
2.2 pix fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits
2.2 pix fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits
Limiting magnitude estimates:
14.9 mag. Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
14.9 mag. Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
13.6 mag. fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits
13.6 mag. fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits
All-image limiting magnitude estimate: 13.6 (SNR ) 13.1 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.2r9RGCfxZX (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/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.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_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits' -> 'wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
WCS_IMAGE_NAME=wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
WCS-calibrated image found: wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
Checking if the catalog wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat corresponding to the image wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits alredy exist and is non-empty...
Catalog wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat corresponding to the image wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
WCS catalog name: wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=34, blended=33174, passed=232827
Got 232827 stars (including 199306 good ones) from the SExtractor catalog wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat
util/solve_plate_with_UCAC5 got 232827 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (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 0.010470 (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 943 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: 0.69"
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 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.69"
Estimated accuracy of the plate solution: 0.63"
Excluding outliers - 941 stars left (next iteration limit 1035)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits -region wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.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.s6KNMSFMGt (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/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.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_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits' -> 'wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
WCS_IMAGE_NAME=wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
WCS-calibrated image found: wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
Checking if the catalog wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat corresponding to the image wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits alredy exist and is non-empty...
Catalog wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat corresponding to the image wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
WCS catalog name: wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=51, blended=32901, passed=232172
Got 232172 stars (including 198927 good ones) from the SExtractor catalog wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat
util/solve_plate_with_UCAC5 got 232172 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.3'
Seting catalog search parameters based on the expected field of view 942.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013088 (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 0.010470 (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 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.70"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.70"
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 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.70"
Estimated accuracy of the plate solution: 0.62"
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_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits -region wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.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.0sUzmGmFco (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_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.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_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits
WCS_IMAGE_NAME=wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits
WCS-calibrated image found: wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits
Checking if the catalog wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits.cat corresponding to the image wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits.cat corresponding to the image wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits
WCS catalog name: wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=13, blended=5543, passed=86094
Got 86094 stars (including 80440 good ones) from the SExtractor catalog wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits.cat
util/solve_plate_with_UCAC5 got 86094 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.5'
Seting catalog search parameters based on the expected field of view 938.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013035 (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 0.010428 (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 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.61"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.59"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.59"
Estimated accuracy of the plate solution: 0.67"
Excluding outliers - 929 stars left (next iteration limit 1021)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits -region wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.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.XQOdtfM6WV (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_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.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_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits
WCS_IMAGE_NAME=wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits
WCS-calibrated image found: wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits
Checking if the catalog wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits.cat corresponding to the image wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits.cat corresponding to the image wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits
WCS catalog name: wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=5762, passed=88168
Got 88168 stars (including 82293 good ones) from the SExtractor catalog wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits.cat
util/solve_plate_with_UCAC5 got 88168 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.4'
Seting catalog search parameters based on the expected field of view 938.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013033 (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 0.010427 (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 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.61"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.59"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.59"
Estimated accuracy of the plate solution: 0.67"
Excluding outliers - 932 stars left (next iteration limit 1025)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits -region wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.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_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.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_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/wcs_Vul-02-Q2b1x1_2026-02-27_05-52-53_20.00sec_-15.00C_LIGHT_0043.fits
Saving fully-calibrated image wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.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_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/wcs_Vul-02-Q2b1x1_2026-02-27_05-53-28_20.00sec_-15.00C_LIGHT_0044.fits
Saving fully-calibrated image wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.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_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-03_20.00sec_-10.00C_LIGHT_0341.fits
Saving fully-calibrated image wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.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_2026-03-30_CI_Vul-02-Q2b1x1_044129_TTUQ2b1x1_10416_TwYe8Cfp/wcs_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342.fits
Preparing the HTML report for the field Vul-02-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out262694.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out262705.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out262720.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out262735.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out262739.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out262742.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out262743.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out262748.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out262755.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out262757.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out262769.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out262795.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out262796.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out262800.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out262801.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out262811.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out262816.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out262834.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out262841.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out263414.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out263680.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out263742.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out263964.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out35019.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out263697.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out263809.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out61062.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 25s
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
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Considering the candidate 262694_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 262694_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:18:54.79 +23:11:44.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)
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Considering the candidate 262698_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 262698_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:34:17.21 +22:11:18.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262704_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 262704_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:17:03.39 +23:58:56.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262705_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 262705_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:22:51.15 +23:53:50.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 2.735 1831884060923824128 305.71379811383 +23.89791783064 13.1958 12.3611 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.735#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262707_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 262707_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:10:42.88 +23:05:52.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262720_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 262720_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:33:03.71 +24:12:29.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 2.078 1831345776954604416 308.26604159679 +24.20850185472 13.1874 12.3894 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.078#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 262735_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 262735_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:11:47.29 +23:00:11.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.11, MAG_FAINT_SEARCH_LIMIT=14.09)
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Considering the candidate 262737_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 262737_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:36:03.10 +23:28:37.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262739_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 262739_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:27:34.44 +25:01:32.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 2.512 1832438524021138944 306.89426876838 +25.02559454167 13.0509 12.2595 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.512#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 262741_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 262741_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:21:02.06 +25:26:01.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262742_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 262742_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 19:55:28.82 +25:03:47.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)
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Considering the candidate 262743_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 262743_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:14:35.02 +17:53:27.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 4.397 1810010720198278272 303.64701601860 +17.89163032300 13.0505 12.5552 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.397#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 262748_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 262748_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:39:12.56 +21:18:14.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.81, MAG_FAINT_SEARCH_LIMIT=13.79)
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Considering the candidate 262755_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 262755_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:37:21.46 +25:35:29.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 2.120 1855608979222633216 309.33996833924 +25.59178703937 12.9923 12.4630 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.120#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 262757_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 262757_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:44:06.39 +25:32:44.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 5.754 1843635503752555008 311.02839594552 +25.54562107309 12.6204 11.8138 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.754#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 262758_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 262758_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:35:57.72 +25:46:40.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262765_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 262765_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:25:27.40 +25:54:09.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262769_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 262769_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:21:28.53 +19:38:03.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.00, MAG_FAINT_SEARCH_LIMIT=13.98)GAIADR2_OUTPUT=# 4.049 1816319855349950336 305.37002935647 +19.63404548437 13.2739 12.5349 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.049#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 262775_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 262775_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:24:46.19 +22:40:16.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262777_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 262777_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:32:35.70 +21:04:58.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262783_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 262783_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:27:22.06 +25:09:52.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262785_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 262785_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:31:06.30 +21:27:09.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262789_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 262789_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:36:25.01 +21:40:21.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262792_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 262792_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:38:34.29 +26:01:45.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262795_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 262795_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 19:57:34.60 +21:45:49.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 4.641 1826902964038935808 299.39535092574 +21.76436681897 12.4632 11.5154 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.641#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262796_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 262796_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 19:58:50.47 +19:37:27.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 3.861 1823069409336841472 299.71081081759 +19.62523228473 12.7741 12.3127 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.861#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262800_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 262800_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 19:59:44.65 +20:34:51.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 1.597 1823750251877484928 299.93644513592 +20.58114933614 12.7960 12.0324 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.597#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262801_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 262801_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:17:34.14 +21:42:13.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.51, MAG_FAINT_SEARCH_LIMIT=13.49)GAIADR2_OUTPUT=# 3.592 1829326528155344768 304.39299374547 +21.70433074497 12.5694 11.9944 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.592#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 262802_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 262802_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:36:30.39 +24:01:43.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262807_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 262807_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:36:29.10 +25:58:59.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262811_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 262811_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 19:53:02.24 +19:09:25.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 5.014 1821684814956390144 298.26075909307 +19.15749427210 12.6338 11.8068 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.014#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 262814_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 262814_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:33:56.86 +22:27:49.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262816_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 262816_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:33:25.88 +20:22:04.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 2.679 1816005012763291776 308.35812094575 +20.36858236273 12.1266 11.4123 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.679#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 262818_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 262818_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:29:18.14 +22:44:13.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262820_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 262820_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:21:04.87 +26:01:18.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262821_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 262821_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:35:47.02 +24:36:29.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262826_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 262826_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 19:56:15.94 +21:01:02.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262827_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 262827_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:40:09.07 +25:16:54.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262834_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 262834_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:28:26.68 +23:57:03.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.63, MAG_FAINT_SEARCH_LIMIT=12.61)GAIADR2_OUTPUT=# 3.527 1831183019178772224 307.11223122783 +23.95071875849 11.7196 10.9498 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.527#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 262838_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 262838_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:41:55.21 +21:36:18.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262839_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 262839_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:27:08.74 +23:11:30.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 262841_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 262841_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:25:39.48 +25:21:12.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.06, MAG_FAINT_SEARCH_LIMIT=11.04)GAIADR2_OUTPUT=# 1.071 1832488689240232320 306.41482468287 +25.35345112881 10.0654 9.8598 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.071#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 263082_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 263082_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:36:06.91 +25:41:10.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263150_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 263150_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:42:59.43 +22:03:19.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263193_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 263193_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:44:16.74 +22:28:21.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263202_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 263202_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:38:30.19 +21:10:10.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 263358_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 263358_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:36:14.64 +22:58:50.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263379_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 263379_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:42:41.37 +25:28:32.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263414_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 263414_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:44:03.27 +21:23:46.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 4.573 1817821925666826368 311.01491398915 +21.39663884822 12.1806 11.6235 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.573#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263445_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 263445_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 19:57:54.49 +20:31:22.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263495_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 263495_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:03:52.04 +21:04:38.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263525_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 263525_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:27:08.06 +20:27:33.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263529_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 263529_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:16:14.08 +21:34:57.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 263557_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 263557_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:36:56.29 +25:41:14.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263567_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 263567_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:18:07.50 +22:30:17.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263576_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 263576_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:11:12.98 +21:52:36.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 263590_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 263590_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:41:56.51 +20:40:13.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263607_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 263607_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 19:50:40.11 +20:12:45.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263647_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 263647_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:20:26.48 +17:48:39.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 263667_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 263667_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 19:53:18.17 +20:20:46.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263680_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 263680_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:14:00.10 +18:37:03.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.73, MAG_FAINT_SEARCH_LIMIT=13.71)GAIADR2_OUTPUT=# 5.662 1810378919155961856 303.50101996301 +18.61910404641 12.9354 12.4099 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.662#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263693_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 263693_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:28:05.10 +19:45:03.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263697_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
Preparing report for the candidate 263697_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
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Considering the candidate 263729_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 263729_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 19:54:00.59 +18:12:17.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263739_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 263739_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:40:42.38 +26:03:17.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263742_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 263742_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:26:57.46 +23:05:05.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.71, MAG_FAINT_SEARCH_LIMIT=13.69)GAIADR2_OUTPUT=# 2.839 1830835844072617344 306.74007228414 +23.08528603837 12.7959 12.2200 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.839#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263779_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 263779_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 19:59:01.71 +23:05:56.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 263809_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
Preparing report for the candidate 263809_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263865_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 263865_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:26:54.05 +24:58:36.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263892_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 263892_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:24:20.09 +25:51:15.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 263934_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 263934_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:40:14.37 +25:47:10.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263935_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 263935_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:22:44.31 +24:03:33.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263950_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 263950_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:36:48.94 +26:00:31.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263961_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 263961_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:10:31.80 +20:57:43.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 263964_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 263964_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:17:17.24 +20:12:57.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 2.094 1828513091399212672 304.32223839665 +20.21539311680 12.9571 12.0327 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.094#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 264045_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 264045_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:09:04.79 +21:38:19.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264062_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 264062_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:20:09.24 +19:55:09.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264100_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 264100_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:17:46.42 +21:07:41.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 264121_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 264121_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:29:29.09 +25:31:55.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 34531_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 34531_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:07:12.44 +18:12:25.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 61062_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
Preparing report for the candidate 61062_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
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Considering the candidate 166677_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 166677_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:42:21.86 +23:43:46.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 176744_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 176744_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 19:56:28.87 +23:54:46.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 35019_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 35019_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:31:16.80 +18:24:29.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.58, MAG_FAINT_SEARCH_LIMIT=13.56)GAIADR2_OUTPUT=# 2.453 1815531363768670848 307.81944833265 +18.40857513755 12.8697 12.7984 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.453#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 149736_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 149736_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 20:11:00.01 +22:51:41.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 60371_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 60371_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks
**** FOUND 19:52:33.28 +19:06:24.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 87318_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342
The candidate 87318_fd_Vul-02-Q2b1x1_2026-03-30_04-40-52_20.00sec_-10.00C_LIGHT_0342 did not pass the final checks