This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d
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 27.3373 2461126.8373 12.79 16:31:46.41 -13:49:49.8
2.58325 22.68322 galactic Oph Second-epoch detections are separated by 1.3" and 9.2 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 4330261176874003328 | 16:31:45.87 -13:49:46.6 (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 4330261176874003328,2461126.8373,12.79,0.05,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 4330261176874003328 20260327.3373 12.79CV 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/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:31:46.41 -13:49:49.8 ;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_Oph-07-Q2b1x1_2026-02-27_06-22-43_20_00sec_-15_00C_LIGHT_0321_fits__*pix.png resample_wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20_00sec_-15_00C_LIGHT_0332_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20_00sec_-15_00C_LIGHT_0321_fits__*pix.png resample_wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20_00sec_-14_90C_LIGHT_0331_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20_00sec_-15_00C_LIGHT_0321_fits__*pix.png resample_wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20_00sec_-15_00C_LIGHT_0332_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20_00sec_-15_00C_LIGHT_0321_fits__*pix.png resample_wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20_00sec_-14_90C_LIGHT_0331_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461126.8373,11.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260327.3373 11.48CV 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/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:50:29.70 -20:30:30.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20_00sec_-15_00C_LIGHT_0321_fits__*pix.png resample_wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20_00sec_-15_00C_LIGHT_0332_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20_00sec_-15_00C_LIGHT_0321_fits__*pix.png resample_wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20_00sec_-14_90C_LIGHT_0331_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20_00sec_-15_00C_LIGHT_0321_fits__*pix.png resample_wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20_00sec_-15_00C_LIGHT_0332_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20_00sec_-15_00C_LIGHT_0321_fits__*pix.png resample_wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20_00sec_-14_90C_LIGHT_0331_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461126.8373,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260327.3373 12.76CV 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/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:27:18.05 -14:23:29.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20_00sec_-15_00C_LIGHT_0321_fits__*pix.png resample_wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20_00sec_-15_00C_LIGHT_0332_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20_00sec_-15_00C_LIGHT_0321_fits__*pix.png resample_wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20_00sec_-14_90C_LIGHT_0331_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20_00sec_-15_00C_LIGHT_0321_fits__*pix.png resample_wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20_00sec_-15_00C_LIGHT_0332_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20_00sec_-15_00C_LIGHT_0321_fits__*pix.png resample_wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20_00sec_-14_90C_LIGHT_0331_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J165420.48-192802.2,2461126.8373,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J165420.48-192802.2 20260327.3373 12.65CV 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/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:54:20.42 -19:28:02.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20_00sec_-15_00C_LIGHT_0321_fits__*pix.png resample_wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20_00sec_-15_00C_LIGHT_0332_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20_00sec_-15_00C_LIGHT_0321_fits__*pix.png resample_wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20_00sec_-14_90C_LIGHT_0331_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20_00sec_-15_00C_LIGHT_0321_fits__*pix.png resample_wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20_00sec_-15_00C_LIGHT_0332_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20_00sec_-15_00C_LIGHT_0321_fits__*pix.png resample_wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20_00sec_-14_90C_LIGHT_0331_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: 2461099.01590147 27.02.2026 12:22:43.887 /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
First image: 2461099.01590147 27.02.2026 12:22:43.887 /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
Last image: 2461126.83761492 27.03.2026 08:05:59.929 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 3
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.41
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 3 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 4461
Objects passed selection criteria: 4443
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 3298
Average stars matched: 3235.75 (98.1125 %)
Memory usage VmPeak: 111548 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 03:08:09 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: 2461099.01590147 27.02.2026 12:22:43.887 /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
First image: 2461099.01590147 27.02.2026 12:22:43.887 /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
Last image: 2461126.83761492 27.03.2026 08:05:59.929 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 43
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.00
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: 10 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): 53648
Objects passed selection criteria: 53547
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: 38413.2
Average stars matched: 36936.2 (96.155 %)
Memory usage VmPeak: 160920 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 03:09:11 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/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits
SExtractor catalog cache: saved Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits.cat to cache
SExtractor catalog cache: saved Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.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/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.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: 2461126.83699603
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_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits exists and is non-empty
Saving wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits to local_wcs_cache/
'wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits' -> 'local_wcs_cache/wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits'
wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits exists and is non-empty
Saving wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits to local_wcs_cache/
'wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits' -> 'local_wcs_cache/wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits'
wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits exists and is non-empty
Saving wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits to local_wcs_cache/
'wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits' -> 'local_wcs_cache/wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits'
wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits exists and is non-empty
Saving wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits to local_wcs_cache/
'wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits' -> 'local_wcs_cache/wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits'
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 16:53:19.722 -18:00:16.64
Second-epoch image center 16:53:21.045 -18:00:18.41
Angular distance between the image centers 0.01 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 16:53:19.722 -18:00:16.64
Second-epoch image center 16:53:23.878 -17:59:44.97
Angular distance between the image centers 0.02 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 16:53:21.045 -18:00:18.41
Second-epoch second image center 16:53:23.878 -17:59:44.97
Angular distance between the image centers 0.01457 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/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits &> /tmp/tmp.Cf1ac38S7t
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits &> /tmp/tmp.3M8u36s65L
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits &> /tmp/tmp.Fr4w62vKuW
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits &> /tmp/tmp.oGO1sVNXBX
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits
Calibrating the magnitude scale
Found non-empty wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.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_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits and wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.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_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits and wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits.cat
Found non-empty wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits and wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits.cat
The reference image (wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits) and catalog (wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits.cat) found
'wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.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 4388 out of 6528 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.922522
a=0.000000 b=1.000000 c=22.922522
From vast_summary.log: estimated ref. image limiting mag.: -8.41
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.51
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.51
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.3 pix Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
2.3 pix Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
3.0 pix fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits
3.0 pix fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits
Limiting magnitude estimates:
14.5 mag. Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
14.5 mag. Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
12.6 mag. fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits
12.6 mag. fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits
All-image limiting magnitude estimate: 12.6 (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.Cf1ac38S7t (6) ############
Parsing command line arguments...
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_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits' -> 'wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
WCS_IMAGE_NAME=wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
WCS-calibrated image found: wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
Checking if the catalog wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits.cat corresponding to the image wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits alredy exist and is non-empty...
Catalog wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits.cat corresponding to the image wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
WCS catalog name: wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=427, passed=6528
Got 6528 stars (including 6093 good ones) from the SExtractor catalog wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits.cat
util/solve_plate_with_UCAC5 got 6528 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 946 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: 0.62"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.64"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.65"
Estimated accuracy of the plate solution: 0.69"
Excluding outliers - 946 stars left (next iteration limit 1040)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits -region wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.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.3M8u36s65L (6) ############
Parsing command line arguments...
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_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits' -> 'wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
WCS_IMAGE_NAME=wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
WCS-calibrated image found: wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
Checking if the catalog wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits.cat corresponding to the image wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits alredy exist and is non-empty...
Catalog wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits.cat corresponding to the image wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
WCS catalog name: wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=428, passed=6260
Got 6260 stars (including 5826 good ones) from the SExtractor catalog wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits.cat
util/solve_plate_with_UCAC5 got 6260 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.62"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.63"
Estimated accuracy of the plate solution: 0.67"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits -region wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.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.Fr4w62vKuW (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_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.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_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits
WCS_IMAGE_NAME=wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits
WCS-calibrated image found: wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits
Checking if the catalog wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits.cat corresponding to the image wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits alredy exist and is non-empty...
Catalog wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits.cat corresponding to the image wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.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_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits
WCS catalog name: wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=70, passed=2150
Got 2150 stars (including 2078 good ones) from the SExtractor catalog wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits.cat
util/solve_plate_with_UCAC5 got 2150 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010430 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.68"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.69"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.69"
Estimated accuracy of the plate solution: 0.67"
Excluding outliers - 942 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_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits -region wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.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.oGO1sVNXBX (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_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.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_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits
WCS_IMAGE_NAME=wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits
WCS-calibrated image found: wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits
Checking if the catalog wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits.cat corresponding to the image wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits alredy exist and is non-empty...
Catalog wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits.cat corresponding to the image wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.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_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits
WCS catalog name: wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=76, passed=2204
Got 2204 stars (including 2128 good ones) from the SExtractor catalog wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits.cat
util/solve_plate_with_UCAC5 got 2204 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.6'
Seting catalog search parameters based on the expected field of view 938.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013036 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010429 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 946 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: 0.68"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.68"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.67"
Estimated accuracy of the plate solution: 0.66"
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_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits -region wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.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_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits'
Saving fully-calibrated image wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits'
Saving fully-calibrated image wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits'
Saving fully-calibrated image wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits'
Preparing the HTML report for the field Oph-07-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
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Considering the candidate 20238_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332
The candidate 20238_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332 did not pass the final checks
**** FOUND 17:05:18.24 -15:36:41.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20075_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332
The candidate 20075_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332 did not pass the final checks
**** FOUND 17:09:35.15 -19:02:15.6 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 0s
Prepared the HTML report for the field Oph-07-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/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits
SExtractor catalog cache: saved Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits.cat to cache
SExtractor catalog cache: saved Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
Creating symlink local_wcs_cache/wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
Creating symlink local_wcs_cache/wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits
Creating symlink local_wcs_cache/wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.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_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits exists and is non-empty
wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits exists and is non-empty
wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits exists and is non-empty
wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits exists and is non-empty
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 16:53:19.722 -18:00:16.64
Second-epoch image center 16:53:21.045 -18:00:18.41
Angular distance between the image centers 0.01 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 16:53:19.722 -18:00:16.64
Second-epoch image center 16:53:23.878 -17:59:44.97
Angular distance between the image centers 0.02 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 16:53:21.045 -18:00:18.41
Second-epoch second image center 16:53:23.878 -17:59:44.97
Angular distance between the image centers 0.01457 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/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits &> /tmp/tmp.o6Ns20zLe1
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits &> /tmp/tmp.xT4sHMhX9h
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits &> /tmp/tmp.gBnX3mF684
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits &> /tmp/tmp.fhsusAoEBb
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits
Calibrating the magnitude scale
Found non-empty wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.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_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits and wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.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_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits and wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits.cat
Found non-empty wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits and wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits.cat
The reference image (wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits) and catalog (wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits.cat) found
'wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.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 5263 out of 75508 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.684879
a=0.000000 b=1.000000 c=22.684879
From vast_summary.log: estimated ref. image limiting mag.: -8.00
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.68
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.68
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 39 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
2.0 pix Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
2.9 pix fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits
3.0 pix fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits
Limiting magnitude estimates:
14.7 mag. Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
14.6 mag. Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
13.3 mag. fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits
13.3 mag. fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits
All-image limiting magnitude estimate: 13.3 (SNR ) 12.8 (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.o6Ns20zLe1 (6) ############
Parsing command line arguments...
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_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits' -> 'wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
WCS_IMAGE_NAME=wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
WCS-calibrated image found: wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
Checking if the catalog wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits.cat corresponding to the image wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits alredy exist and is non-empty...
Catalog wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits.cat corresponding to the image wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
WCS catalog name: wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=4239, passed=75506
Got 75506 stars (including 71154 good ones) from the SExtractor catalog wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits.cat
util/solve_plate_with_UCAC5 got 75506 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.60"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.60"
Estimated accuracy of the plate solution: 0.64"
Excluding outliers - 942 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_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits -region wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.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.xT4sHMhX9h (6) ############
Parsing command line arguments...
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_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits' -> 'wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
WCS_IMAGE_NAME=wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
WCS-calibrated image found: wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
Checking if the catalog wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits.cat corresponding to the image wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits alredy exist and is non-empty...
Catalog wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits.cat corresponding to the image wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
WCS catalog name: wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=3, blended=4544, passed=72943
Got 72943 stars (including 68297 good ones) from the SExtractor catalog wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits.cat
util/solve_plate_with_UCAC5 got 72943 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 941 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: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.57"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.57"
Estimated accuracy of the plate solution: 0.61"
Excluding outliers - 941 stars left (next iteration limit 1035)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits -region wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.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.gBnX3mF684 (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_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.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_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits
WCS_IMAGE_NAME=wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits
WCS-calibrated image found: wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits
Checking if the catalog wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits.cat corresponding to the image wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits alredy exist and is non-empty...
Catalog wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits.cat corresponding to the image wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.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_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits
WCS catalog name: wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=509, passed=18766
Got 18766 stars (including 18243 good ones) from the SExtractor catalog wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits.cat
util/solve_plate_with_UCAC5 got 18766 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.7'
Seting catalog search parameters based on the expected field of view 938.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013038 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010430 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.67"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.64"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.64"
Estimated accuracy of the plate solution: 0.62"
Excluding outliers - 945 stars left (next iteration limit 1040)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits -region wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.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.fhsusAoEBb (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_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.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_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits
WCS_IMAGE_NAME=wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits
WCS-calibrated image found: wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits
Checking if the catalog wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits.cat corresponding to the image wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits alredy exist and is non-empty...
Catalog wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits.cat corresponding to the image wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.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_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits
WCS catalog name: wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=500, passed=18775
Got 18775 stars (including 18253 good ones) from the SExtractor catalog wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits.cat
util/solve_plate_with_UCAC5 got 18775 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 938.6'
Seting catalog search parameters based on the expected field of view 938.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013036 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010429 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.62"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 946 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.62"
Estimated accuracy of the plate solution: 0.61"
Excluding outliers - 946 stars left (next iteration limit 1040)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits -region wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.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_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.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_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/wcs_Oph-07-Q2b1x1_2026-02-27_06-22-43_20.00sec_-15.00C_LIGHT_0321.fits
Saving fully-calibrated image wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.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_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/wcs_Oph-07-Q2b1x1_2026-02-27_06-23-33_20.00sec_-15.00C_LIGHT_0322.fits
Saving fully-calibrated image wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.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_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-06_20.00sec_-14.90C_LIGHT_0331.fits
Saving fully-calibrated image wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.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_Oph-07-Q2b1x1_030648_TTUQ2b1x1_6519_PW5ZZA4d/wcs_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332.fits
Preparing the HTML report for the field Oph-07-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_local.txt__out28804.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out91305.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out91318.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out91344.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 14s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 91305_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332
Preparing report for the candidate 91305_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332
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Considering the candidate 91318_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332
Preparing report for the candidate 91318_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 91337_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332
The candidate 91337_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332 did not pass the final checks
**** FOUND 16:40:40.30 -20:24:45.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 91342_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332
The candidate 91342_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332 did not pass the final checks
**** FOUND 16:48:20.12 -15:22:14.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 91344_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332
Preparing report for the candidate 91344_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332
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Considering the candidate 35334_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332
The candidate 35334_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332 did not pass the final checks
**** FOUND 16:27:01.51 -18:27:21.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 09667_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332
The candidate 09667_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332 did not pass the final checks
**** FOUND 16:32:08.25 -21:27:56.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 42583_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332
The candidate 42583_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332 did not pass the final checks
**** FOUND 16:41:34.49 -17:44:32.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 68777_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332
The candidate 68777_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332 did not pass the final checks
**** FOUND 17:05:18.23 -15:36:41.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 48442_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332
The candidate 48442_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332 did not pass the final checks
**** FOUND 16:46:55.68 -17:18:46.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 29642_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332
The candidate 29642_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332 did not pass the final checks
**** FOUND 17:03:36.95 -19:22:48.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 36865_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332
The candidate 36865_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332 did not pass the final checks
**** FOUND 16:26:10.07 -18:23:14.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 32447_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332
The candidate 32447_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332 did not pass the final checks
**** FOUND 17:09:35.13 -19:02:15.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 47737_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332
The candidate 47737_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332 did not pass the final checks
**** FOUND 17:16:18.78 -17:23:37.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23203_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332
The candidate 23203_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332 did not pass the final checks
**** FOUND 16:46:39.49 -20:03:26.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 28804_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332
Preparing report for the candidate 28804_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332
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Considering the candidate 68030_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332
The candidate 68030_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332 did not pass the final checks
**** FOUND 17:15:09.96 -15:17:51.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 27735_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332
The candidate 27735_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332 did not pass the final checks
**** FOUND 16:49:02.48 -19:27:50.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 35782_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332
The candidate 35782_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332 did not pass the final checks
**** FOUND 17:15:30.08 -18:40:29.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65028_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332
The candidate 65028_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332 did not pass the final checks
**** FOUND 17:12:33.11 -14:52:45.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 68062_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332
The candidate 68062_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332 did not pass the final checks
**** FOUND 17:12:55.12 -15:18:07.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 38986_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332
The candidate 38986_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332 did not pass the final checks
**** FOUND 16:49:55.04 -18:20:51.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 27431_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332
The candidate 27431_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332 did not pass the final checks
**** FOUND 17:04:35.55 -19:38:01.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 26578_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332
The candidate 26578_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332 did not pass the final checks
**** FOUND 16:57:03.84 -19:32:23.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 32194_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332
The candidate 32194_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332 did not pass the final checks
**** FOUND 17:01:51.07 -18:53:07.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 67945_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332
The candidate 67945_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332 did not pass the final checks
**** FOUND 17:13:01.55 -15:16:45.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 19279_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332
The candidate 19279_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332 did not pass the final checks
**** FOUND 16:53:25.13 -20:24:55.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 10220_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332
The candidate 10220_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332 did not pass the final checks
**** FOUND 16:55:32.51 -21:34:09.6 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 44619_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332
The candidate 44619_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332 did not pass the final checks
**** FOUND 17:08:14.70 -17:36:30.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 18582_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332
The candidate 18582_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332 did not pass the final checks
**** FOUND 17:04:45.28 -20:29:40.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 23245_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332
The candidate 23245_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332 did not pass the final checks
**** FOUND 16:41:53.79 -19:55:25.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 18481_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332
The candidate 18481_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332 did not pass the final checks
**** FOUND 16:40:34.57 -20:24:29.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 10219_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332
The candidate 10219_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332 did not pass the final checks
**** FOUND 17:06:11.77 -21:33:54.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 70469_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332
The candidate 70469_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332 did not pass the final checks
**** FOUND 17:10:22.46 -15:43:28.2 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 67381_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332
The candidate 67381_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332 did not pass the final checks
**** FOUND 17:16:15.74 -15:13:26.1 in the exclusion list exclusion_list_tycho2.txt ****
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Considering the candidate 74023_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332
The candidate 74023_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332 did not pass the final checks
**** FOUND 17:18:19.07 -16:18:43.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 61783_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332
The candidate 61783_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332 did not pass the final checks
**** FOUND 17:15:20.21 -14:35:03.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 20421_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332
The candidate 20421_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332 did not pass the final checks
**** FOUND 16:24:06.30 -20:02:13.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 61596_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332
The candidate 61596_fd_Oph-07-Q2b1x1_2026-03-27_03-05-59_20.00sec_-15.00C_LIGHT_0332 did not pass the final checks