This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L
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 27.3598 2461126.8598 12.31 19:00:23.29 +25:25:01.0
56.73224 9.45802 galactic Vul Second-epoch detections are separated by 2.2" and 6.9 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 4533956975926747136 | 19:00:23.13 +25:24:52.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
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 4533956975926747136,2461126.8598,12.31,0.05,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 4533956975926747136 20260327.3598 12.31CV 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-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:00:23.29 +25:25:01.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20_00sec_-14_90C_LIGHT_0359_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20_00sec_-14_90C_LIGHT_0358_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20_00sec_-14_90C_LIGHT_0359_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20_00sec_-14_90C_LIGHT_0358_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.3598 2461126.8598 12.04 19:08:20.35 +21:02:03.5
53.58167 5.88091 galactic Sge Second-epoch detections are separated by 5.9" and 6.4 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 4519795128729797632 | 19:08:18.62 +21:01:36.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
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 4519795128729797632,2461126.8598,12.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 4519795128729797632 20260327.3598 12.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:08:20.35 +21:02:03.5 ;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-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20_00sec_-14_90C_LIGHT_0359_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20_00sec_-14_90C_LIGHT_0358_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20_00sec_-14_90C_LIGHT_0359_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20_00sec_-14_90C_LIGHT_0358_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 27.3598 2461126.8598 11.96 19:46:00.20 +22:55:06.0
59.39909 -0.90303 galactic Vul Second-epoch detections are separated by 1.7" and 7.8 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 1827882422731442944 | 19:45:58.94 +22:55:23.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.511+/-0.058 (K)
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 1827882422731442944,2461126.8598,11.96,0.05,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 1827882422731442944 20260327.3598 11.96CV 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-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:46:00.20 +22:55:06.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20_00sec_-14_90C_LIGHT_0359_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20_00sec_-14_90C_LIGHT_0358_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20_00sec_-14_90C_LIGHT_0359_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20_00sec_-14_90C_LIGHT_0358_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
FL Aql,2461126.8598,11.77,0.05,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
FL Aql 20260327.3598 11.77CV 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-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:05:01.03 +18:02:42.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20_00sec_-14_90C_LIGHT_0359_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20_00sec_-14_90C_LIGHT_0358_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20_00sec_-14_90C_LIGHT_0359_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20_00sec_-15_00C_LIGHT_0041_fits__*pix.png resample_wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20_00sec_-14_90C_LIGHT_0358_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: 2461098.99380530 27.02.2026 11:50:54.778 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
First image: 2461098.99380530 27.02.2026 11:50:54.778 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
Last image: 2461126.86011707 27.03.2026 08:38:24.115 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits
JD time system (TT/UTC/UNKNOWN): UTC
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.87
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): 17329
Objects passed selection criteria: 17229
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 11866.8
Average stars matched: 11540.2 (97.2486 %)
Memory usage VmPeak: 124060 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 Fri Mar 27 03:45:41 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: 2461098.99380530 27.02.2026 11:50:54.778 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
First image: 2461098.99380530 27.02.2026 11:50:54.778 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
Last image: 2461126.86011707 27.03.2026 08:38:24.115 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 101
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.54
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: 26 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): 170955
Objects passed selection criteria: 170466
Measurements per detected object (mean, median, min, max): 2.4 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.4 2.0 2 4
Average stars detected per image: 111515
Average stars matched: 105611 (94.7054 %)
Memory usage VmPeak: 2269908 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 Fri Mar 27 03:50:12 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-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits
SExtractor catalog cache: saved Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat to cache
SExtractor catalog cache: saved Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.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-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461126.85951829
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-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits exists and is non-empty
Saving wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits to local_wcs_cache/
'wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits' -> 'local_wcs_cache/wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits'
wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits exists and is non-empty
Saving wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits to local_wcs_cache/
'wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits' -> 'local_wcs_cache/wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits'
wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits exists and is non-empty
Saving wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits to local_wcs_cache/
'wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits' -> 'local_wcs_cache/wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits'
wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits exists and is non-empty
Saving wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits to local_wcs_cache/
'wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits' -> 'local_wcs_cache/wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.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 19:23:05.554 +21:59:47.51
Second-epoch image center 19:23:09.362 +21:57:23.40
Angular distance between the image centers 0.04 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 19:23:05.554 +21:59:47.51
Second-epoch image center 19:23:06.990 +21:56:50.99
Angular distance between the image centers 0.05 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 19:23:09.362 +21:57:23.40
Second-epoch second image center 19:23:06.990 +21:56:50.99
Angular distance between the image centers 0.01285 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-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits &> /tmp/tmp.H8bqWHeye7
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits &> /tmp/tmp.4LU2d3vGmB
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits &> /tmp/tmp.rAO5519KtB
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits &> /tmp/tmp.HhkFLrpmkH
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits
Calibrating the magnitude scale
Found non-empty wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.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-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits and wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.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-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits and wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat
Found non-empty wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits and wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat
The reference image (wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits) and catalog (wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat) found
'wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.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 14431 out of 24236 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.881026
a=0.000000 b=1.000000 c=22.881026
From vast_summary.log: estimated ref. image limiting mag.: -7.87
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.01
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.01
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 0 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
2.2 pix Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
4.9 pix fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits
3.4 pix fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits
Limiting magnitude estimates:
15.0 mag. Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
15.0 mag. Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
13.1 mag. fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits
13.4 mag. fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits
All-image limiting magnitude estimate: 13.1 (SNR ) 10.6 (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.H8bqWHeye7 (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-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.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_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.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-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.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-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits' -> 'wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
WCS_IMAGE_NAME=wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
WCS-calibrated image found: wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
Checking if the catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat corresponding to the image wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits alredy exist and is non-empty...
Catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat corresponding to the image wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
WCS catalog name: wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat
SExtractor catalog parsing summary: zero_flux=4, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2379, passed=24232
Got 24232 stars (including 21810 good ones) from the SExtractor catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat
util/solve_plate_with_UCAC5 got 24232 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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 963 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: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.44"
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 962 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.44"
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits -region wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.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.4LU2d3vGmB (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-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.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_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.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-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.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-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits' -> 'wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
WCS_IMAGE_NAME=wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
WCS-calibrated image found: wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
Checking if the catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat corresponding to the image wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits alredy exist and is non-empty...
Catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat corresponding to the image wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
WCS catalog name: wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2427, passed=23940
Got 23940 stars (including 21482 good ones) from the SExtractor catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat
util/solve_plate_with_UCAC5 got 23940 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
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 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.48"
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits -region wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.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.rAO5519KtB (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_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.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_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits
WCS_IMAGE_NAME=wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits
WCS-calibrated image found: wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits
Checking if the catalog wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits
WCS catalog name: wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=119, passed=4822
Got 4822 stars (including 4702 good ones) from the SExtractor catalog wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits.cat
util/solve_plate_with_UCAC5 got 4822 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.0'
Seting catalog search parameters based on the expected field of view 939.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013042 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010433 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 950 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.89"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.92"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.93"
Estimated accuracy of the plate solution: 0.99"
Excluding outliers - 945 stars left (next iteration limit 1039)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits -region wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.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.HhkFLrpmkH (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_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.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_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits
WCS_IMAGE_NAME=wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits
WCS-calibrated image found: wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits
Checking if the catalog wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits
WCS catalog name: wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=227, passed=6789
Got 6789 stars (including 6553 good ones) from the SExtractor catalog wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits.cat
util/solve_plate_with_UCAC5 got 6789 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.0'
Seting catalog search parameters based on the expected field of view 939.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013042 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010433 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.77"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.79"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.80"
Estimated accuracy of the plate solution: 0.88"
Excluding outliers - 943 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits -region wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.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-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits'
Saving fully-calibrated image wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits'
Saving fully-calibrated image wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits'
Saving fully-calibrated image wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits'
Preparing the HTML report for the field Vul-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Vul-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits
SExtractor catalog cache: saved Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat to cache
SExtractor catalog cache: saved Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.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-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
Creating symlink local_wcs_cache/wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
Creating symlink local_wcs_cache/wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits
Creating symlink local_wcs_cache/wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.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-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits exists and is non-empty
wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits exists and is non-empty
wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits exists and is non-empty
wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.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 19:23:05.554 +21:59:47.51
Second-epoch image center 19:23:09.362 +21:57:23.40
Angular distance between the image centers 0.04 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 19:23:05.554 +21:59:47.51
Second-epoch image center 19:23:06.990 +21:56:50.99
Angular distance between the image centers 0.05 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 19:23:09.362 +21:57:23.40
Second-epoch second image center 19:23:06.990 +21:56:50.99
Angular distance between the image centers 0.01285 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-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits &> /tmp/tmp.ac9gMiLbcF
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits &> /tmp/tmp.l5vb6A25ln
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits &> /tmp/tmp.Ltu9l9c8h0
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits &> /tmp/tmp.SR13bQ4AFA
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits
Calibrating the magnitude scale
Found non-empty wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.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-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits and wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.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-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits and wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat
Found non-empty wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits and wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat
The reference image (wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits) and catalog (wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat) found
'wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.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 15518 out of 221580 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.709941
a=0.000000 b=1.000000 c=22.709941
From vast_summary.log: estimated ref. image limiting mag.: -7.54
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.17
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.17
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 67 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
1.9 pix Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
4.9 pix fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits
3.4 pix fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits
Limiting magnitude estimates:
15.2 mag. Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
15.2 mag. Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
13.1 mag. fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits
13.5 mag. fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits
All-image limiting magnitude estimate: 13.1 (SNR ) 12.4 (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.ac9gMiLbcF (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-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.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_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.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-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.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-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits' -> 'wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
WCS_IMAGE_NAME=wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
WCS-calibrated image found: wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
Checking if the catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat corresponding to the image wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits alredy exist and is non-empty...
Catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat corresponding to the image wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
WCS catalog name: wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat
SExtractor catalog parsing summary: zero_flux=1, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=40, blended=30047, passed=221539
Got 221539 stars (including 191094 good ones) from the SExtractor catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat
util/solve_plate_with_UCAC5 got 221539 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.44"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.46"
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 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.46"
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits -region wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.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.l5vb6A25ln (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-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.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_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.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-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.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-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits' -> 'wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
WCS_IMAGE_NAME=wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
WCS-calibrated image found: wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
Checking if the catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat corresponding to the image wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits alredy exist and is non-empty...
Catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat corresponding to the image wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
WCS catalog name: wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=41, blended=30936, passed=228140
Got 228140 stars (including 196813 good ones) from the SExtractor catalog wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat
util/solve_plate_with_UCAC5 got 228140 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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 965 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: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.52"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.52"
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 963 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits -region wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.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.Ltu9l9c8h0 (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_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.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_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits
WCS_IMAGE_NAME=wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits
WCS-calibrated image found: wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits
Checking if the catalog wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits
WCS catalog name: wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=1688, passed=27084
Got 27084 stars (including 25376 good ones) from the SExtractor catalog wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits.cat
util/solve_plate_with_UCAC5 got 27084 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.0'
Seting catalog search parameters based on the expected field of view 939.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013042 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010433 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 947 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.88"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.90"
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 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.90"
Estimated accuracy of the plate solution: 0.95"
Excluding outliers - 941 stars left (next iteration limit 1036)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits -region wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.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.SR13bQ4AFA (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_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.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_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits
WCS_IMAGE_NAME=wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits
WCS-calibrated image found: wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits
Checking if the catalog wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits alredy exist and is non-empty...
Catalog wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits.cat corresponding to the image wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits
WCS catalog name: wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=2515, passed=45668
Got 45668 stars (including 43097 good ones) from the SExtractor catalog wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits.cat
util/solve_plate_with_UCAC5 got 45668 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.0'
Seting catalog search parameters based on the expected field of view 939.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013042 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010433 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 949 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.75"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.71"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 950 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.71"
Estimated accuracy of the plate solution: 0.77"
Excluding outliers - 945 stars left (next iteration limit 1039)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits -region wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.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-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.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_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/wcs_Vul-01-Q2b1x1_2026-02-27_05-50-54_20.00sec_-15.00C_LIGHT_0041.fits
Saving fully-calibrated image wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.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_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/wcs_Vul-01-Q2b1x1_2026-02-27_05-51-50_20.00sec_-14.90C_LIGHT_0042.fits
Saving fully-calibrated image wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.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_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-37-32_20.00sec_-14.90C_LIGHT_0358.fits
Saving fully-calibrated image wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.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_2026-03-27_CI_Vul-01-Q2b1x1_034207_TTUQ2b1x1_28423_HOdw4w4L/wcs_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359.fits
Preparing the HTML report for the field Vul-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out234264.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254440.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254441.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254442.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254444.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254445.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254446.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254448.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254450.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254451.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254452.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out254455.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out254457.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out254461.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out254465.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out30752.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 15s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 254440_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 254440_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:15:46.82 +19:45:32.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.58, MAG_FAINT_SEARCH_LIMIT=13.56)GAIADR2_OUTPUT=# 1.366 4516251162249314688 288.94548330601 +19.75901969313 12.3374 11.6115 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.366#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254441_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 254441_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:23:32.04 +24:06:11.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.67, MAG_FAINT_SEARCH_LIMIT=13.65)GAIADR2_OUTPUT=# 1.640 2022778688447614720 290.88384737024 +24.10286739835 12.2820 11.3549 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.640#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254442_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 254442_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:20:15.20 +19:41:12.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.40, MAG_FAINT_SEARCH_LIMIT=13.38)GAIADR2_OUTPUT=# 1.726 4515806650304714752 290.06342326029 +19.68627814056 12.2146 11.6148 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.726#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254444_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 254444_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:47:18.00 +21:09:18.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 1.430 1827352423775508608 296.82457663426 +21.15503968582 11.7274 11.2866 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.430#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254445_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 254445_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:44:26.82 +20:32:12.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 0.729 1825816229894638976 296.11181011582 +20.53666665821 11.5249 10.5017 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.729#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254446_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 254446_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:39:53.74 +22:29:23.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 1.508 2019936897563888128 294.97437000128 +22.48986821676 12.0981 11.5836 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.508#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254448_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 254448_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:31:59.58 +25:40:09.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 4.318 2024534097470805760 292.99951606391 +25.66970281362 11.4699 10.3692 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.318#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254450_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 254450_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:14:38.08 +26:00:32.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 2.407 2024183933026275456 288.65801990854 +26.00855839788 11.7611 10.8436 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.407#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254451_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 254451_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 18:53:41.54 +25:03:23.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.44, MAG_FAINT_SEARCH_LIMIT=13.42)GAIADR2_OUTPUT=# 0.716 4534272604481467904 283.42326131451 +25.05658876456 12.5704 12.2426 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.716#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254452_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 254452_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:48:19.64 +22:02:45.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 3.520 1827573082016432000 297.08181585035 +22.04694998971 11.4360 10.4513 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.520#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254455_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 254455_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 18:56:10.02 +24:26:32.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.42, MAG_FAINT_SEARCH_LIMIT=13.40)GAIADR2_OUTPUT=# 2.587 4533432264050141824 284.04253943753 +24.44227470279 12.1094 11.3179 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.587#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 254457_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
Preparing report for the candidate 254457_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
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Considering the candidate 254461_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
Preparing report for the candidate 254461_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
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Considering the candidate 254465_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
Preparing report for the candidate 254465_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
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Considering the candidate 254474_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 254474_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 254477_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 254477_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:15:54.45 +22:59:12.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 254802_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 254802_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:07:57.80 +21:42:42.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 121912_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 121912_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:45:37.53 +22:51:12.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 177832_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 177832_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:02:34.31 +25:50:26.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 30752_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
Preparing report for the candidate 30752_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
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Considering the candidate 52335_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 52335_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:27:53.53 +19:17:37.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 150311_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 150311_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:43:58.79 +24:09:39.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234337_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 234337_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:46:16.49 +20:22:01.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 234264_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 234264_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:20:33.38 +17:45:56.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.63, MAG_FAINT_SEARCH_LIMIT=11.61)
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Considering the candidate 110128_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 110128_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 18:58:11.48 +21:52:54.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 112797_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 112797_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:35:41.45 +22:20:08.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 82475_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 82475_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:12:25.06 +20:39:01.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 182417_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 182417_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:28:47.36 +25:53:05.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 140690_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 140690_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:39:20.34 +23:44:18.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 96854_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 96854_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:48:41.60 +21:33:35.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105210_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 105210_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:17:31.96 +21:48:51.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 117889_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 117889_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:17:39.98 +22:26:27.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 75358_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 75358_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:23:12.23 +20:16:42.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 74738_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 74738_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:27:54.04 +20:14:50.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 112215_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 112215_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:20:54.35 +22:11:55.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 104274_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 104274_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:33:25.54 +21:50:19.8 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 62768_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 62768_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:18:48.39 +19:36:38.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 74206_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 74206_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:26:30.66 +20:15:33.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 74955_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 74955_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:25:22.39 +20:16:17.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 121209_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 121209_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:19:32.03 +22:34:14.3 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 74870_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 74870_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:23:46.94 +20:15:52.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 52153_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 52153_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:20:59.90 +19:08:46.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 74394_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 74394_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:29:20.93 +20:16:47.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 118172_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 118172_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:36:08.42 +22:35:08.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 33657_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 33657_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:27:26.64 +18:17:44.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 75620_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 75620_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:15:02.81 +20:12:12.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 101612_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 101612_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:12:36.91 +21:33:17.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 170317_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 170317_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:25:25.48 +24:54:29.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 83562_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 83562_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:38:17.77 +20:46:58.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 166026_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 166026_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:28:57.16 +24:46:08.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 106317_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 106317_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:08:03.73 +21:41:59.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 47866_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 47866_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:35:07.61 +19:00:17.4 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 156680_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 156680_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:08:37.86 +24:10:44.9 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 98333_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 98333_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:03:42.52 +21:16:06.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 46953_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 46953_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:37:23.44 +18:58:35.2 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 41097_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 41097_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:15:33.45 +18:31:00.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 116362_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 116362_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:41:14.64 +22:27:09.4 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 123511_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 123511_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:42:48.49 +22:51:04.7 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 117927_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 117927_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:01:49.64 +22:15:51.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 159112_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 159112_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:06:38.63 +24:15:03.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 55929_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 55929_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:04:52.66 +19:08:40.0 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 60420_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 60420_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:01:05.53 +19:18:34.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 70643_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 70643_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 18:58:45.10 +19:47:39.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 193572_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 193572_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:47:48.80 +25:23:02.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 67608_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 67608_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 19:02:52.76 +19:39:40.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 131782_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 131782_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks
**** FOUND 18:59:58.31 +22:48:52.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 184740_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359
The candidate 184740_fd_Vul-01-Q2b1x1_2026-03-27_03-38-24_20.00sec_-14.90C_LIGHT_0359 did not pass the final checks