This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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
BK Dra,2461124.9819,10.38,0.05,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
BK Dra 20260325.4819 10.38CV 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/Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:18:20.59 +66:24:48.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20_00sec_-15_00C_LIGHT_0209_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20_00sec_-15_00C_LIGHT_0209_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20_00sec_-15_00C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20_00sec_-15_00C_LIGHT_0209_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20_00sec_-15_00C_LIGHT_0209_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20_00sec_-15_00C_LIGHT_0211_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 25.4819 2461124.9819 12.69 19:37:25.28 +70:24:57.2
102.22545 21.72499 galactic Dra Second-epoch detections are separated by 3.5" and 1.7 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 2263182370372871168 | 19:37:21.41 +70:24:30.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0V 1948UppAn...2d....S BD+70 1079 J-Ks=0.440+/-0.085 (G)
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 2263182370372871168,2461124.9819,12.69,0.05,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 2263182370372871168 20260325.4819 12.69CV 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/Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:37:25.28 +70:24:57.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20_00sec_-15_00C_LIGHT_0209_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20_00sec_-15_00C_LIGHT_0209_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20_00sec_-15_00C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20_00sec_-15_00C_LIGHT_0209_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20_00sec_-15_00C_LIGHT_0209_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20_00sec_-15_00C_LIGHT_0211_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461124.9819,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260325.4819 13.46CV 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/Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 18:55:25.22 +67:23:42.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20_00sec_-15_00C_LIGHT_0209_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20_00sec_-15_00C_LIGHT_0209_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20_00sec_-15_00C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20_00sec_-15_00C_LIGHT_0209_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20_00sec_-15_00C_LIGHT_0209_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20_00sec_-15_00C_LIGHT_0211_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
NR Dra,2461124.9819,13.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NR Dra 20260325.4819 13.07CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 19:49:53.85 +68:10:19.9 ;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_Dra-05-Q2b1x1_2026-03-19_06-10-12_20_00sec_-15_00C_LIGHT_0209_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20_00sec_-15_00C_LIGHT_0209_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20_00sec_-15_00C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20_00sec_-15_00C_LIGHT_0209_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20_00sec_-15_00C_LIGHT_0209_fits__*pix.png resample_wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20_00sec_-15_00C_LIGHT_0211_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: 2461118.96554069 19.03.2026 11:10:12.716 /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits
First image: 2461118.96554069 19.03.2026 11:10:12.716 /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits
Last image: 2461124.98217813 25.03.2026 11:34:10.190 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.68
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: 5 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): 11598
Objects passed selection criteria: 11558
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.9 2.0 2 4
Average stars detected per image: 8791.5
Average stars matched: 8624.5 (98.1004 %)
Memory usage VmPeak: 118028 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 Wed Mar 25 06:37:18 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: 2461118.96554069 19.03.2026 11:10:12.716 /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits
First image: 2461118.96554069 19.03.2026 11:10:12.716 /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits
Last image: 2461124.98217813 25.03.2026 11:34:10.190 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 100
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.35
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: 43 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): 70225
Objects passed selection criteria: 70068
Measurements per detected object (mean, median, min, max): 3.1 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.1 4.0 2 4
Average stars detected per image: 57903.2
Average stars matched: 56182.5 (97.0282 %)
Memory usage VmPeak: 1922000 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 Wed Mar 25 06:38:50 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/Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits
SExtractor catalog cache: saved Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits.cat to cache
SExtractor catalog cache: saved Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.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/Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.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: 2461124.98165023
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits exists and is non-empty
Saving wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits to local_wcs_cache/
'wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits' -> 'local_wcs_cache/wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits'
wcs_Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits exists and is non-empty
Saving wcs_Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits to local_wcs_cache/
'wcs_Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits' -> 'local_wcs_cache/wcs_Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits'
wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits exists and is non-empty
Saving wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits to local_wcs_cache/
'wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits' -> 'local_wcs_cache/wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits'
wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits exists and is non-empty
Saving wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits to local_wcs_cache/
'wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits' -> 'local_wcs_cache/wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.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 19:12:02.913 +70:00:00.99
Second-epoch image center 19:12:01.740 +70:00:32.37
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 19:12:02.913 +70:00:00.99
Second-epoch image center 19:12:03.501 +70:00:41.26
Angular distance between the image centers 0.01 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 19:12:01.740 +70:00:32.37
Second-epoch second image center 19:12:03.501 +70:00:41.26
Angular distance between the image centers 0.00352 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/Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits &> /tmp/tmp.7HZrDPoG60
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits &> /tmp/tmp.tjjBZZUj9N
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits &> /tmp/tmp.bkoq9RDPFd
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits &> /tmp/tmp.VwvOvZxH1N
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits
Calibrating the magnitude scale
Found non-empty wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.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_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits and wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.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_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits and wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits.cat
Found non-empty wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits and wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits.cat
The reference image (wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits) and catalog (wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits.cat) found
'wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.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 8263 out of 14881 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.888382
a=0.000000 b=1.000000 c=22.888382
From vast_summary.log: estimated ref. image limiting mag.: -7.68
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.21
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.21
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.4 pix Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits
2.4 pix Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits
2.3 pix fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits
2.3 pix fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits
Limiting magnitude estimates:
15.2 mag. Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits
15.2 mag. Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits
14.1 mag. fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits
14.0 mag. fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 11.3 (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.7HZrDPoG60 (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_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits' -> 'wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits
WCS_IMAGE_NAME=wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits
WCS-calibrated image found: wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits
Checking if the catalog wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits.cat corresponding to the image wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits alredy exist and is non-empty...
Catalog wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits.cat corresponding to the image wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits
WCS catalog name: wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits.cat
SExtractor catalog parsing summary: zero_flux=4, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=963, passed=14877
Got 14877 stars (including 13902 good ones) from the SExtractor catalog wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits.cat
util/solve_plate_with_UCAC5 got 14877 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 969 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: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.49"
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits -region wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.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.tjjBZZUj9N (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_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits' -> 'wcs_Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits
WCS_IMAGE_NAME=wcs_Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits
WCS-calibrated image found: wcs_Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits
Checking if the catalog wcs_Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits.cat corresponding to the image wcs_Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits alredy exist and is non-empty...
Catalog wcs_Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits.cat corresponding to the image wcs_Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits
WCS catalog name: wcs_Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=988, passed=14811
Got 14811 stars (including 13810 good ones) from the SExtractor catalog wcs_Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits.cat
util/solve_plate_with_UCAC5 got 14811 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 968 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: 0.52"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.51"
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 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.51"
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits -region wcs_Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.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.bkoq9RDPFd (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_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.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_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits
WCS_IMAGE_NAME=wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits
WCS-calibrated image found: wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits
Checking if the catalog wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits.cat corresponding to the image wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits alredy exist and is non-empty...
Catalog wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits.cat corresponding to the image wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits
WCS catalog name: wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=319, passed=6632
Got 6632 stars (including 6303 good ones) from the SExtractor catalog wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits.cat
util/solve_plate_with_UCAC5 got 6632 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.49"
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits -region wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.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.VwvOvZxH1N (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_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.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_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits
WCS_IMAGE_NAME=wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits
WCS-calibrated image found: wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits
Checking if the catalog wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits.cat corresponding to the image wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits alredy exist and is non-empty...
Catalog wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits.cat corresponding to the image wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits
WCS catalog name: wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=318, passed=6558
Got 6558 stars (including 6232 good ones) from the SExtractor catalog wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits.cat
util/solve_plate_with_UCAC5 got 6558 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
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 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.48"
Estimated accuracy of the plate solution: 0.51"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits -region wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.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_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits'
Saving fully-calibrated image wcs_Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/wcs_Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits'
Saving fully-calibrated image wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits'
Saving fully-calibrated image wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits'
Preparing the HTML report for the field Dra-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out03085.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 4s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03085_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 03085_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 5s
Prepared the HTML report for the field Dra-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
19:18:20.59 +66:24:48.5
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/Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits
SExtractor catalog cache: saved Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits.cat to cache
SExtractor catalog cache: saved Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits
Creating symlink local_wcs_cache/wcs_Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits
Creating symlink local_wcs_cache/wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits
Creating symlink local_wcs_cache/wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.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_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits exists and is non-empty
wcs_Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits exists and is non-empty
wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits exists and is non-empty
wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.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 19:12:02.913 +70:00:00.99
Second-epoch image center 19:12:01.740 +70:00:32.37
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 19:12:02.913 +70:00:00.99
Second-epoch image center 19:12:03.501 +70:00:41.26
Angular distance between the image centers 0.01 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 19:12:01.740 +70:00:32.37
Second-epoch second image center 19:12:03.501 +70:00:41.26
Angular distance between the image centers 0.00352 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/Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits &> /tmp/tmp.lOQd3uD6n6
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits &> /tmp/tmp.YApCvPdnr5
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits &> /tmp/tmp.cy2hJLEAVs
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits &> /tmp/tmp.wDFUQHNVKk
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits
Calibrating the magnitude scale
Found non-empty wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.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_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits and wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.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_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits and wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits.cat
Found non-empty wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits and wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits.cat
The reference image (wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits) and catalog (wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits.cat) found
'wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.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 8406 out of 86853 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.743933
a=0.000000 b=1.000000 c=22.743933
From vast_summary.log: estimated ref. image limiting mag.: -7.35
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.39
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.39
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 77 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits
2.2 pix Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits
2.1 pix fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits
2.2 pix fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits
Limiting magnitude estimates:
15.4 mag. Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits
15.4 mag. Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits
14.3 mag. fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits
14.3 mag. fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 13.8 (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.lOQd3uD6n6 (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_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits' -> 'wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits
WCS_IMAGE_NAME=wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits
WCS-calibrated image found: wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits
Checking if the catalog wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits.cat corresponding to the image wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits alredy exist and is non-empty...
Catalog wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits.cat corresponding to the image wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits
WCS catalog name: wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits.cat
SExtractor catalog parsing summary: zero_flux=5, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=27, blended=6611, passed=86821
Got 86821 stars (including 80106 good ones) from the SExtractor catalog wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits.cat
util/solve_plate_with_UCAC5 got 86821 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 973 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: 0.51"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.49"
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits -region wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.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.YApCvPdnr5 (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_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits' -> 'wcs_Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits
WCS_IMAGE_NAME=wcs_Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits
WCS-calibrated image found: wcs_Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits
Checking if the catalog wcs_Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits.cat corresponding to the image wcs_Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits alredy exist and is non-empty...
Catalog wcs_Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits.cat corresponding to the image wcs_Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits
WCS catalog name: wcs_Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=20, blended=6554, passed=87123
Got 87123 stars (including 80460 good ones) from the SExtractor catalog wcs_Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits.cat
util/solve_plate_with_UCAC5 got 87123 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 972 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: 0.52"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.50"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 972 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.50"
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 972 stars left (next iteration limit 1069)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits -region wcs_Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.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.cy2hJLEAVs (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_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.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_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits
WCS_IMAGE_NAME=wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits
WCS-calibrated image found: wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits
Checking if the catalog wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits.cat corresponding to the image wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits alredy exist and is non-empty...
Catalog wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits.cat corresponding to the image wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits
WCS catalog name: wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=1942, passed=46004
Got 46004 stars (including 44007 good ones) from the SExtractor catalog wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits.cat
util/solve_plate_with_UCAC5 got 46004 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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 966 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: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.47"
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits -region wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.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.wDFUQHNVKk (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_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.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_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits
WCS_IMAGE_NAME=wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits
WCS-calibrated image found: wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits
Checking if the catalog wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits.cat corresponding to the image wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits alredy exist and is non-empty...
Catalog wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits.cat corresponding to the image wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits
WCS catalog name: wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=1950, passed=44999
Got 44999 stars (including 42989 good ones) from the SExtractor catalog wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits.cat
util/solve_plate_with_UCAC5 got 44999 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.4'
Seting catalog search parameters based on the expected field of view 937.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013019 (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 0.010416 (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 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.46"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.46"
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits -region wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.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_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.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_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/wcs_Dra-05-Q2b1x1_2026-03-19_06-10-12_20.00sec_-15.00C_LIGHT_0209.fits
Saving fully-calibrated image wcs_Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.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_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/wcs_Dra-05-Q2b1x1_2026-03-19_06-11-23_20.00sec_-14.90C_LIGHT_0210.fits
Saving fully-calibrated image wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.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_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-33-24_20.00sec_-15.00C_LIGHT_0211.fits
Saving fully-calibrated image wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.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_2026-03-25_CI_Dra-05-Q2b1x1_063459_TTUQ2b1x1_30107_X18CgW03/wcs_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212.fits
Preparing the HTML report for the field Dra-05-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out103299.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103301.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103305.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103307.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103311.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103314.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103368.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103394.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103423.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103424.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103430.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103436.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103444.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103450.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103452.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103464.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103473.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103474.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103480.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103484.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103531.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103534.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103535.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103537.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103552.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103556.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103560.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103585.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103591.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103611.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out103407.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out103510.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35168.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 16s
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
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Considering the candidate 103299_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103299_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 19:00:31.60 +72:56:23.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 1.285 2267601105744127488 285.13287286383 +72.93976946484 13.7519 13.2086 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.285#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103301_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103301_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 18:53:00.85 +71:10:47.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 0.588 2265881572636391936 283.25373912354 +71.17962724798 13.6221 13.5737 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.588#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103305_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103305_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 19:06:51.51 +66:30:32.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 0.485 2255741567168442880 286.71496093717 +66.50890203630 13.6578 13.1297 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.485#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103307_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103307_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 18:48:09.15 +72:19:06.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 0.690 2266104532979320576 282.03803227086 +72.31825474725 13.1655 12.4281 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.690#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103311_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103311_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 19:14:49.11 +66:57:14.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)GAIADR2_OUTPUT=# 0.574 2255062962336031488 288.70484515953 +66.95405065172 13.7694 13.3598 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.574#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103314_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103314_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 19:06:37.18 +70:05:05.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.28, MAG_FAINT_SEARCH_LIMIT=13.26)GAIADR2_OUTPUT=# 0.786 2262213704926313216 286.65555427487 +70.08488359098 12.2356 11.7146 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.786#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103368_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103368_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 19:32:35.58 +69:36:40.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.08, MAG_FAINT_SEARCH_LIMIT=13.06)GAIADR2_OUTPUT=# 0.221 2261611103834350848 293.14816795803 +69.61127644951 11.9552 11.2071 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.221#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103377_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103377_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 103378_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103378_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
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Considering the candidate 103383_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103383_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
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Considering the candidate 103394_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103394_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 18:06:11.99 +72:34:44.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 2.519 2266827049556948608 271.55205319644 +72.57863434701 12.6117 12.5766 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.519#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103405_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103405_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 103407_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 103407_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 103408_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103408_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 20:02:48.77 +67:50:22.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 103409_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103409_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 20:05:22.22 +73:26:04.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103423_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103423_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 19:49:08.55 +65:58:26.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 1.133 2248573026234425344 297.28588322569 +65.97432450023 13.1280 12.6812 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.133#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103424_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103424_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 18:12:03.94 +66:09:36.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 0.627 2257559918882106624 273.01680695721 +66.16024030781 12.8795 12.4150 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.627#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103430_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103430_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 20:00:52.83 +71:20:23.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 0.744 2251682960513140352 300.21948907108 +71.33979722720 13.0609 12.5030 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.744#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103436_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103436_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 19:23:14.33 +68:59:47.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 0.350 2261673638558692608 290.80983722294 +68.99672439164 13.1219 12.6128 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.350#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103437_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103437_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
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Considering the candidate 103444_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103444_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 19:57:47.63 +71:55:54.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 0.873 2251764083855662464 299.44903445851 +71.93199736288 12.8715 12.1036 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.873#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103450_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103450_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 19:11:19.94 +66:59:45.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 0.766 2255030698542426880 287.83362113422 +66.99597842469 13.3667 12.8670 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.766#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103451_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103451_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (13.8") between the two second-epoch detections
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Considering the candidate 103452_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103452_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 19:41:01.10 +67:44:42.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.19, MAG_FAINT_SEARCH_LIMIT=14.17)GAIADR2_OUTPUT=# 0.990 2249339832513858816 295.25528560691 +67.74515321141 13.3605 12.8364 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.990#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103453_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103453_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 18:28:14.78 +73:45:25.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103454_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103454_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 103455_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103455_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 103460_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103460_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 103464_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103464_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 18:53:55.92 +67:06:17.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 0.963 2255653846757139968 283.48354796490 +67.10472734074 13.2572 12.5777 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.963#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103466_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103466_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 18:19:25.73 +71:31:08.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103467_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103467_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 18:15:11.52 +68:43:57.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 103473_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103473_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 19:26:45.64 +73:21:45.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 2.074 2264862424140902784 291.68817969272 +73.36260374016 13.3868 12.9914 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.074#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103474_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103474_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 19:49:22.97 +65:56:31.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 1.648 2248572751356503040 297.34682557626 +65.94212845627 13.3032 12.7504 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.648#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103480_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103480_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 20:07:39.43 +71:25:55.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.30, MAG_FAINT_SEARCH_LIMIT=14.28)GAIADR2_OUTPUT=# 0.596 2251696910567138176 301.91419384323 +71.43200403179 13.4122 12.6641 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.596#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103484_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103484_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 19:46:51.79 +66:46:12.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 2.156 2248681774806832896 296.71699082358 +66.77045069199 13.6398 13.0056 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.156#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103487_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103487_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 103490_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103490_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 103496_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103496_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 103497_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103497_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 103507_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103507_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 103510_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 103510_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 103523_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103523_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 103530_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103530_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 103531_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103531_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 19:31:45.42 +67:43:21.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 4.304 2260976582546003456 292.94031602681 +67.72368087472 13.9178 13.3907 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.304#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103533_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103533_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
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Considering the candidate 103534_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103534_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 18:04:14.44 +67:54:11.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 1.539 2258357545848389888 271.05975839195 +67.90345457470 14.4868 13.7662 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.539#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103535_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103535_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 18:13:31.57 +65:17:59.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 0.686 2161419893459115392 273.38156976936 +65.29975433285 13.3305 12.2794 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.686#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103537_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103537_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 19:24:05.45 +72:33:45.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 1.267 2264392662094031616 291.02321423079 +72.56221028777 13.1503 12.6857 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.267#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103542_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103542_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 19:31:22.61 +70:59:25.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 103545_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103545_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 103547_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103547_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 103552_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103552_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 19:00:59.24 +71:20:54.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 1.885 2262899417927568128 285.24659600016 +71.34806529602 13.5204 12.9293 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.885#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103555_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103555_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 103556_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103556_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 18:58:33.25 +74:06:28.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 0.681 2267771186449303808 284.63912209329 +74.10770276419 13.6743 13.1288 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.681#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103557_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103557_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 103560_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103560_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 18:56:34.18 +68:17:36.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 1.038 2256182436970782592 284.14298849220 +68.29377949483 13.9235 13.7683 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.038#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103566_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103566_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 103572_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103572_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 103573_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103573_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
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Considering the candidate 103578_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103578_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 103579_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103579_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 103584_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103584_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 19:56:19.11 +70:06:17.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 103585_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103585_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 19:15:18.05 +73:14:03.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 3.160 2264659053145653760 288.82373107241 +73.23359370067 13.8736 13.2804 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.160#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103587_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103587_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 103588_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103588_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
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Considering the candidate 103591_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103591_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 19:29:53.39 +70:55:45.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)GAIADR2_OUTPUT=# 1.624 2263445845143866752 292.47280371084 +70.92884098229 14.1058 13.5467 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.624#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103597_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103597_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 103603_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103603_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 103605_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103605_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 103608_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103608_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 103611_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103611_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 18:47:34.65 +66:51:33.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 1.766 2255586295512075392 281.89487872841 +66.85967116093 14.0304 13.4340 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.766#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 103627_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103627_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
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Considering the candidate 103632_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103632_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 103634_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 103634_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 24656_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 24656_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 15257_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212
The candidate 15257_fd_Dra-05-Q2b1x1_2026-03-25_06-34-10_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks