This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR
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
ASAS J090621-2856.3,2461125.6324,11.58,0.05,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
ASAS J090621-2856.3 20260326.1324 11.58CV 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/Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:06:21.88 -28:56:15.9 ;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_Ant-01-Q2b1x1_2026-01-09_02-36-03_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20_00sec_-10_00C_LIGHT_0319_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20_00sec_-10_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20_00sec_-10_00C_LIGHT_0319_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20_00sec_-10_00C_LIGHT_0318_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 26.1324* 09 46 57.80 -27 38 16.2 11.6 U Ant 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
SV Ant,2461125.6324,11.62,0.05,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
SV Ant 20260326.1324 11.62CV 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/Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:46:57.80 -27:38:16.2 ;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_Ant-01-Q2b1x1_2026-01-09_02-36-03_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20_00sec_-10_00C_LIGHT_0319_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20_00sec_-10_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20_00sec_-10_00C_LIGHT_0319_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20_00sec_-10_00C_LIGHT_0318_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
AZ Hya,2461125.6324,9.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
AZ Hya 20260326.1324 9.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:45:36.21 -23:53:51.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20_00sec_-10_00C_LIGHT_0319_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20_00sec_-10_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20_00sec_-10_00C_LIGHT_0319_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20_00sec_-10_00C_LIGHT_0318_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 26.1324* 10 00 42.65 -27 43 28.6 12.5 U Ant 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J100043-2743.5,2461125.6324,12.49,0.05,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
ASAS J100043-2743.5 20260326.1324 12.49CV 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/Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 10:00:42.65 -27:43:28.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20_00sec_-10_00C_LIGHT_0319_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20_00sec_-10_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20_00sec_-10_00C_LIGHT_0319_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20_00sec_-15_00C_LIGHT_0013_fits__*pix.png resample_wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20_00sec_-10_00C_LIGHT_0318_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: 2461049.85848940 09.01.2026 08:36:03.484 /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits
First image: 2461049.85848940 09.01.2026 08:36:03.484 /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits
Last image: 2461125.63264927 26.03.2026 03:10:50.897 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 13
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -8.26
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 8072
Objects passed selection criteria: 8070
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 7897.75
Average stars matched: 7179.75 (90.9088 %)
Memory usage VmPeak: 114608 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 22:15:20 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: 2461049.85848940 09.01.2026 08:36:03.484 /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits
First image: 2461049.85848940 09.01.2026 08:36:03.484 /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits
Last image: 2461125.63264927 26.03.2026 03:10:50.897 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 56
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.94
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: 29 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): 61968
Objects passed selection criteria: 61884
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 58592
Average stars matched: 53842.8 (91.8944 %)
Memory usage VmPeak: 166780 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 22:16:30 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/Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits
SExtractor catalog cache: saved Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits.cat to cache
SExtractor catalog cache: saved Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.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/Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.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: 2461125.63209519
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_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits exists and is non-empty
Saving wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits to local_wcs_cache/
'wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits' -> 'local_wcs_cache/wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits'
wcs_Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits exists and is non-empty
Saving wcs_Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits to local_wcs_cache/
'wcs_Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits' -> 'local_wcs_cache/wcs_Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits'
wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits exists and is non-empty
Saving wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits to local_wcs_cache/
'wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits' -> 'local_wcs_cache/wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits'
wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits exists and is non-empty
Saving wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits to local_wcs_cache/
'wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits' -> 'local_wcs_cache/wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:36:02.540 -25:59:22.87
Second-epoch image center 09:36:00.895 -26:00:51.05
Angular distance between the image centers 0.03 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 09:36:02.540 -25:59:22.87
Second-epoch image center 09:36:00.901 -26:00:20.01
Angular distance between the image centers 0.02 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 09:36:00.895 -26:00:51.05
Second-epoch second image center 09:36:00.901 -26:00:20.01
Angular distance between the image centers 0.00862 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/Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits &> /tmp/tmp.jp6Ps4NVfM
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits &> /tmp/tmp.uBr6DAttGa
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits &> /tmp/tmp.sDMC2PNfSZ
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits &> /tmp/tmp.fKqgjZekHU
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits
Calibrating the magnitude scale
Found non-empty wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.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_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits and wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.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_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits and wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits.cat
Found non-empty wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits and wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits.cat
The reference image (wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits) and catalog (wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits.cat) found
'wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.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 7443 out of 9358 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.835745
a=0.000000 b=1.000000 c=22.835745
From vast_summary.log: estimated ref. image limiting mag.: -8.26
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.58
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.58
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 6 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits
2.1 pix Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits
2.7 pix fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits
2.7 pix fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits
Limiting magnitude estimates:
14.6 mag. Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits
14.7 mag. Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits
14.2 mag. fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits
14.2 mag. fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits
All-image limiting magnitude estimate: 14.2 (SNR ) 11.4 (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.jp6Ps4NVfM (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits' -> 'wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits
WCS_IMAGE_NAME=wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits
WCS-calibrated image found: wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits
Checking if the catalog wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits.cat corresponding to the image wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits alredy exist and is non-empty...
Catalog wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits.cat corresponding to the image wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits
WCS catalog name: wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=768, passed=9358
Got 9358 stars (including 8573 good ones) from the SExtractor catalog wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits.cat
util/solve_plate_with_UCAC5 got 9358 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 955 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: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.29"
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 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.29"
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 956 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits -region wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.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.uBr6DAttGa (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits' -> 'wcs_Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits
WCS_IMAGE_NAME=wcs_Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits
WCS-calibrated image found: wcs_Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits
Checking if the catalog wcs_Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits.cat corresponding to the image wcs_Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits alredy exist and is non-empty...
Catalog wcs_Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits.cat corresponding to the image wcs_Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits
WCS catalog name: wcs_Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=852, passed=11175
Got 11175 stars (including 10306 good ones) from the SExtractor catalog wcs_Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits.cat
util/solve_plate_with_UCAC5 got 11175 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 958 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: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
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 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits -region wcs_Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.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.sDMC2PNfSZ (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_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.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_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits
WCS_IMAGE_NAME=wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits
WCS-calibrated image found: wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits
Checking if the catalog wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits.cat corresponding to the image wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits alredy exist and is non-empty...
Catalog wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits.cat corresponding to the image wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.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_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits
WCS catalog name: wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=519, passed=8180
Got 8180 stars (including 7654 good ones) from the SExtractor catalog wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits.cat
util/solve_plate_with_UCAC5 got 8180 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.60"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.60"
Estimated accuracy of the plate solution: 0.66"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits -region wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.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.fKqgjZekHU (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_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.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_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits
WCS_IMAGE_NAME=wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits
WCS-calibrated image found: wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits
Checking if the catalog wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits.cat corresponding to the image wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits alredy exist and is non-empty...
Catalog wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits.cat corresponding to the image wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.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_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits
WCS catalog name: wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=541, passed=8172
Got 8172 stars (including 7618 good ones) from the SExtractor catalog wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits.cat
util/solve_plate_with_UCAC5 got 8172 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.62"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.62"
Estimated accuracy of the plate solution: 0.68"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits -region wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.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_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits'
Saving fully-calibrated image wcs_Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/wcs_Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits'
Saving fully-calibrated image wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits'
Saving fully-calibrated image wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits'
Preparing the HTML report for the field Ant-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out22770.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out22774.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out22772.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22761_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319
The candidate 22761_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319 did not pass the final checks
**** FOUND 09:09:28.87 -22:13:08.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22770_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319
The candidate 22770_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319 did not pass the final checks
**** FOUND 09:08:04.46 -23:21:48.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.59, MAG_FAINT_SEARCH_LIMIT=12.57)GAIADR2_OUTPUT=# 0.469 5651817528609989888 137.01844150101 -23.36333416741 11.4700 10.9735 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.469#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22772_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319
Preparing report for the candidate 22772_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22773_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319
The candidate 22773_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319 did not pass the final checks
**** FOUND 09:14:49.43 -26:41:28.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22774_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319
The candidate 22774_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319 did not pass the final checks
**** FOUND 09:05:45.06 -25:08:07.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.65, MAG_FAINT_SEARCH_LIMIT=12.63)GAIADR2_OUTPUT=# 0.194 5651000557110948096 136.43769056920 -25.13528183002 11.3112 10.4391 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.194#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 01198_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319
The candidate 01198_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319 did not pass the final checks
**** FOUND 09:26:35.03 -30:03:18.7 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 5s
Prepared the HTML report for the field Ant-01-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
09:06:21.88 -28:56:15.9
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/Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits
SExtractor catalog cache: saved Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits.cat to cache
SExtractor catalog cache: saved Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits
Creating symlink local_wcs_cache/wcs_Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits
Creating symlink local_wcs_cache/wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits
Creating symlink local_wcs_cache/wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.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_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits exists and is non-empty
wcs_Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits exists and is non-empty
wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits exists and is non-empty
wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:36:02.540 -25:59:22.87
Second-epoch image center 09:36:00.895 -26:00:51.05
Angular distance between the image centers 0.03 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 09:36:02.540 -25:59:22.87
Second-epoch image center 09:36:00.901 -26:00:20.01
Angular distance between the image centers 0.02 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 09:36:00.895 -26:00:51.05
Second-epoch second image center 09:36:00.901 -26:00:20.01
Angular distance between the image centers 0.00862 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/Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits &> /tmp/tmp.nBPEPKXDFs
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits &> /tmp/tmp.Gjiq78vDIe
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits &> /tmp/tmp.TKpsGPet5b
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits &> /tmp/tmp.3RDBnNJCTb
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits
Calibrating the magnitude scale
Found non-empty wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.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_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits and wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.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_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits and wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits.cat
Found non-empty wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits and wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits.cat
The reference image (wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits) and catalog (wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits.cat) found
'wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.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 9614 out of 74592 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.674802
a=0.000000 b=1.000000 c=22.674802
From vast_summary.log: estimated ref. image limiting mag.: -7.94
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.73
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.73
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 36 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.8 pix Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits
2.0 pix Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits
2.4 pix fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits
2.4 pix fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits
Limiting magnitude estimates:
14.7 mag. Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits
14.9 mag. Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits
14.3 mag. fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits
14.3 mag. fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 13.7 (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.nBPEPKXDFs (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits' -> 'wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits
WCS_IMAGE_NAME=wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits
WCS-calibrated image found: wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits
Checking if the catalog wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits.cat corresponding to the image wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits alredy exist and is non-empty...
Catalog wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits.cat corresponding to the image wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits
WCS catalog name: wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=3863, passed=74584
Got 74584 stars (including 70593 good ones) from the SExtractor catalog wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits.cat
util/solve_plate_with_UCAC5 got 74584 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 955 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: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
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 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.32"
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 955 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits -region wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.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.Gjiq78vDIe (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits' -> 'wcs_Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits
WCS_IMAGE_NAME=wcs_Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits
WCS-calibrated image found: wcs_Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits
Checking if the catalog wcs_Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits.cat corresponding to the image wcs_Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits alredy exist and is non-empty...
Catalog wcs_Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits.cat corresponding to the image wcs_Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits
WCS catalog name: wcs_Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=4995, passed=82266
Got 82266 stars (including 77106 good ones) from the SExtractor catalog wcs_Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits.cat
util/solve_plate_with_UCAC5 got 82266 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 957 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: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
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 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.35"
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits -region wcs_Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.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.TKpsGPet5b (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_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.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_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits
WCS_IMAGE_NAME=wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits
WCS-calibrated image found: wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits
Checking if the catalog wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits.cat corresponding to the image wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits alredy exist and is non-empty...
Catalog wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits.cat corresponding to the image wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.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_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits
WCS catalog name: wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=3147, passed=52365
Got 52365 stars (including 49165 good ones) from the SExtractor catalog wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits.cat
util/solve_plate_with_UCAC5 got 52365 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 953 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: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.54"
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 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.54"
Estimated accuracy of the plate solution: 0.58"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits -region wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.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.3RDBnNJCTb (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_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.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_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits
WCS_IMAGE_NAME=wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits
WCS-calibrated image found: wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits
Checking if the catalog wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits.cat corresponding to the image wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits alredy exist and is non-empty...
Catalog wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits.cat corresponding to the image wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.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_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits
WCS catalog name: wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=3217, passed=52886
Got 52886 stars (including 49598 good ones) from the SExtractor catalog wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits.cat
util/solve_plate_with_UCAC5 got 52886 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.62"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.57"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.57"
Estimated accuracy of the plate solution: 0.62"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-25_CI_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits -region wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.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_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.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_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/wcs_Ant-01-Q2b1x1_2026-01-09_02-36-03_20.00sec_-15.00C_LIGHT_0013.fits
Saving fully-calibrated image wcs_Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.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_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/wcs_Ant-01-Q2b1x1_2026-01-21_02-54-45_20.00sec_-14.90C_LIGHT_0422.fits
Saving fully-calibrated image wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.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_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-03_20.00sec_-10.00C_LIGHT_0318.fits
Saving fully-calibrated image wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.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_Ant-01-Q2b1x1_221306_TTUQ2b1x1_8866_SaobJaNR/wcs_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319.fits
Preparing the HTML report for the field Ant-01-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out102973.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out102974.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out102977.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out102979.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out102986.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out102992.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out102995.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out102997.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out102999.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103001.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103025.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103077.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103089.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103102.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103120.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103138.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103151.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103191.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103195.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out103211.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out26113.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27213.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69699.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102973_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319
The candidate 102973_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319 did not pass the final checks
**** FOUND 09:24:17.09 -22:03:26.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)GAIADR2_OUTPUT=# 0.209 5675463934914104832 141.07124639961 -22.05732378049 14.1284 13.6502 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.209#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102974_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319
The candidate 102974_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319 did not pass the final checks
**** FOUND 09:52:08.38 -30:07:56.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 3.416 5464210127305756672 148.03591258843 -30.13199050539 12.8098 12.0839 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.416#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102977_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319
The candidate 102977_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319 did not pass the final checks
**** FOUND 09:10:35.19 -21:38:28.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 2.059 5679063770343213696 137.64605610918 -21.64094902226 14.0268 13.5555 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.059#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102979_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319
The candidate 102979_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319 did not pass the final checks
**** FOUND 09:27:38.17 -28:19:39.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 2.267 5636838022712715904 141.90931501730 -28.32694589799 13.8713 13.1797 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.267#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102982_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319
The candidate 102982_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319 did not pass the final checks
**** FOUND 09:12:15.09 -21:47:23.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102986_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319
The candidate 102986_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319 did not pass the final checks
**** FOUND 09:11:40.23 -25:15:07.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 0.956 5650246910609583360 137.91764382246 -25.25192934704 13.6077 12.9087 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.956#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102990_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319
The candidate 102990_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319 did not pass the final checks
**** FOUND 09:11:07.04 -23:33:50.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102992_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319
The candidate 102992_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319 did not pass the final checks
**** FOUND 09:15:59.71 -27:54:38.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 3.900 5637466943363829632 138.99971457795 -27.91140768862 13.4176 12.6752 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.900#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102995_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319
The candidate 102995_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319 did not pass the final checks
**** FOUND 09:33:01.66 -27:29:29.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 0.816 5633994101526822528 143.25692209732 -27.49138452369 13.3674 12.8227 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.816#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102997_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319
The candidate 102997_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319 did not pass the final checks
**** FOUND 09:29:01.13 -29:24:05.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)GAIADR2_OUTPUT=# 0.710 5633352983169216512 142.25490746501 -29.40167723534 13.1132 12.7076 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.710#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102999_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319
The candidate 102999_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319 did not pass the final checks
**** FOUND 09:16:17.37 -25:46:00.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 2.023 5650334558006685184 139.07283335425 -25.76713133788 13.2670 12.7219 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.023#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103001_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319
The candidate 103001_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319 did not pass the final checks
**** FOUND 09:44:13.91 -24:07:48.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.03, MAG_FAINT_SEARCH_LIMIT=14.01)GAIADR2_OUTPUT=# 0.301 5663349825036903296 146.05795452032 -24.13013901149 12.9767 12.4492 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.301#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103025_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319
The candidate 103025_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319 did not pass the final checks
**** FOUND 09:21:32.54 -26:00:22.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 0.275 5638270823801194496 140.38550249353 -26.00633736025 11.9000 11.1576 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.275#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103027_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319
The candidate 103027_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319 did not pass the final checks
**** FOUND 09:46:46.89 -28:41:19.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103040_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319
The candidate 103040_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319 did not pass the final checks
**** FOUND 09:26:56.19 -26:23:15.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103067_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319
The candidate 103067_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319 did not pass the final checks
**** FOUND 09:54:16.74 -25:54:29.3 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103069_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319
The candidate 103069_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319 did not pass the final checks
**** FOUND 09:32:41.37 -27:26:23.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103077_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319
The candidate 103077_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319 did not pass the final checks
**** FOUND 09:40:33.55 -23:22:21.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 2.170 5663636557053345280 145.13991056093 -23.37323157243 13.5197 12.9668 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.170#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103089_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319
The candidate 103089_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319 did not pass the final checks
**** FOUND 09:12:02.59 -24:06:27.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 2.287 5651507500690268928 138.01139404957 -24.10806815345 13.9802 13.3910 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.287#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103094_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319
The candidate 103094_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319 did not pass the final checks
**** FOUND 09:16:05.46 -23:39:21.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103102_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319
The candidate 103102_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319 did not pass the final checks
**** FOUND 09:25:14.39 -28:59:28.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 0.105 5636404398516085248 141.30996878102 -28.99113906775 13.3309 12.6642 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.105#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103103_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319
The candidate 103103_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319 did not pass the final checks
**** FOUND 09:33:37.76 -25:45:15.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103116_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319
The candidate 103116_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319 did not pass the final checks
**** FOUND 09:38:09.73 -26:23:25.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103120_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319
The candidate 103120_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319 did not pass the final checks
**** FOUND 09:04:56.22 -28:02:48.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 0.810 5648156567208816512 136.23443942994 -28.04681734281 14.1422 13.6089 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.810#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103138_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319
The candidate 103138_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319 did not pass the final checks
**** FOUND 09:07:52.31 -23:46:11.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 1.716 5651753825655044352 136.96743833145 -23.76980454258 13.8029 13.1311 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.716#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103151_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319
The candidate 103151_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319 did not pass the final checks
**** FOUND 09:10:46.12 -21:40:52.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)GAIADR2_OUTPUT=# 0.392 5679060467511731456 137.69218136769 -21.68105871814 14.1188 13.6044 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.392#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103191_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319
The candidate 103191_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319 did not pass the final checks
**** FOUND 09:37:37.55 -22:01:55.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)GAIADR2_OUTPUT=# 2.327 5664739401575931008 144.40682250856 -22.03161543278 14.5520 14.0046 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.327#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103195_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319
The candidate 103195_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319 did not pass the final checks
**** FOUND 09:23:52.85 -23:42:12.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 0.654 5674605422491136768 140.97011407174 -23.70371553835 14.1831 13.4783 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.654#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 103211_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319
The candidate 103211_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319 did not pass the final checks
**** FOUND 09:24:01.97 -24:58:00.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.24, MAG_FAINT_SEARCH_LIMIT=15.22)GAIADR2_OUTPUT=# 0.610 5662455269248966528 141.00834934657 -24.96658337478 14.3741 13.8960 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.610#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27213_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319
Preparing report for the candidate 27213_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 59245_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319
The candidate 59245_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319 did not pass the final checks
**** FOUND 09:09:28.92 -22:13:08.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08262_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319
The candidate 08262_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319 did not pass the final checks
**** FOUND 09:26:35.02 -30:03:19.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11360_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319
The candidate 11360_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319 did not pass the final checks
**** FOUND 09:35:23.04 -29:44:05.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 43972_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319
The candidate 43972_fd_Ant-01-Q2b1x1_2026-03-25_22-10-50_20.00sec_-10.00C_LIGHT_0319 did not pass the final checks