This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry
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
DG Peg,2461126.9883,10.68,0.05,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
DG Peg 20260327.4883 10.68CV 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/Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:03:33.93 +14:00:30.7 ;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_Peg-09-Q2b1x1_2025-12-22_19-50-17_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20_00sec_-15_00C_LIGHT_0558_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20_00sec_-14_90C_LIGHT_0557_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20_00sec_-15_00C_LIGHT_0558_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20_00sec_-14_90C_LIGHT_0557_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
AB Peg,2461126.9883,10.70,0.05,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
AB Peg 20260327.4883 10.70CV 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/Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:21:58.16 +13:46:38.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20_00sec_-15_00C_LIGHT_0558_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20_00sec_-14_90C_LIGHT_0557_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20_00sec_-15_00C_LIGHT_0558_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20_00sec_-14_90C_LIGHT_0557_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
IU Peg,2461126.9883,11.81,0.05,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
IU Peg 20260327.4883 11.81CV 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/Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:07:16.38 +11:53:16.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20_00sec_-15_00C_LIGHT_0558_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20_00sec_-14_90C_LIGHT_0557_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20_00sec_-15_00C_LIGHT_0558_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20_00sec_-14_90C_LIGHT_0557_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
T Peg,2461126.9883,10.85,0.05,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
T Peg 20260327.4883 10.85CV 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/Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 22:08:54.38 +12:32:23.9 ;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_Peg-09-Q2b1x1_2025-12-22_19-50-17_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20_00sec_-15_00C_LIGHT_0558_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20_00sec_-14_90C_LIGHT_0557_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20_00sec_-15_00C_LIGHT_0558_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20_00sec_-14_90C_LIGHT_0008_fits__*pix.png resample_wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20_00sec_-14_90C_LIGHT_0557_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: 2461032.57670620 23.12.2025 01:50:17.416 /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits
First image: 2461032.57670620 23.12.2025 01:50:17.416 /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits
Last image: 2461126.98856095 27.03.2026 11:43:21.666 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 2
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.70
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 5 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 9518
Objects passed selection criteria: 9462
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 6225.5
Average stars matched: 5943.5 (95.4702 %)
Memory usage VmPeak: 115660 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Mar 27 07:36:04 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: 2461032.57670620 23.12.2025 01:50:17.416 /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits
First image: 2461032.57670620 23.12.2025 01:50:17.416 /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits
Last image: 2461126.98856095 27.03.2026 11:43:21.666 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 16
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.38
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: 30 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): 61085
Objects passed selection criteria: 60897
Measurements per detected object (mean, median, min, max): 2.5 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.5 2.0 2 4
Average stars detected per image: 41072
Average stars matched: 38710 (94.2491 %)
Memory usage VmPeak: 162248 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Fri Mar 27 07:37:36 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/Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits
SExtractor catalog cache: saved Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits.cat to cache
SExtractor catalog cache: saved Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.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/Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461126.98806102
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Plate-solving the images
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits exists and is non-empty
Saving wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits to local_wcs_cache/
'wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits' -> 'local_wcs_cache/wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits'
wcs_Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits exists and is non-empty
Saving wcs_Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits to local_wcs_cache/
'wcs_Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits' -> 'local_wcs_cache/wcs_Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits'
wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits exists and is non-empty
Saving wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits to local_wcs_cache/
'wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits' -> 'local_wcs_cache/wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits'
wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits exists and is non-empty
Saving wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits to local_wcs_cache/
'wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits' -> 'local_wcs_cache/wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.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 22:13:37.402 +13:59:12.14
Second-epoch image center 22:13:40.188 +13:59:18.21
Angular distance between the image centers 0.01 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 22:13:37.402 +13:59:12.14
Second-epoch image center 22:13:40.124 +13:59:13.72
Angular distance between the image centers 0.01 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 22:13:40.188 +13:59:18.21
Second-epoch second image center 22:13:40.124 +13:59:13.72
Angular distance between the image centers 0.00127 deg.
###################################
ERROR: no shift applied between second-epoch images! The distance between image centers is 0.00127 deg. (min. required shift: 0.00164 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/Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits &> /tmp/tmp.uPwYm3BBDX
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits &> /tmp/tmp.6iXMpvUruh
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits &> /tmp/tmp.eB8wwtYERS
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits &> /tmp/tmp.do7kkc4CpN
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits
Calibrating the magnitude scale
Found non-empty wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.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_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits and wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.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_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits and wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits.cat
Found non-empty wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits and wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits.cat
The reference image (wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits) and catalog (wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits.cat) found
'wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.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 6770 out of 11705 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.913070
a=0.000000 b=1.000000 c=22.913070
From vast_summary.log: estimated ref. image limiting mag.: -7.70
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.21
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.21
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 2 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits
2.1 pix Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits
2.8 pix fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits
2.8 pix fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits
Limiting magnitude estimates:
15.2 mag. Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits
15.2 mag. Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits
13.4 mag. fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits
13.4 mag. fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits
All-image limiting magnitude estimate: 13.4 (SNR ) 10.8 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.uPwYm3BBDX (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/Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits' -> 'wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits
WCS_IMAGE_NAME=wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits
WCS-calibrated image found: wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits
Checking if the catalog wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits.cat corresponding to the image wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits alredy exist and is non-empty...
Catalog wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits.cat corresponding to the image wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits
WCS catalog name: wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits.cat
SExtractor catalog parsing summary: zero_flux=6, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=805, passed=11699
Got 11699 stars (including 10873 good ones) from the SExtractor catalog wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits.cat
util/solve_plate_with_UCAC5 got 11699 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 927 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: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
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 927 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.30"
Estimated accuracy of the plate solution: 0.29"
Excluding outliers - 927 stars left (next iteration limit 1019)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits -region wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.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.6iXMpvUruh (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/Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits' -> 'wcs_Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits
WCS_IMAGE_NAME=wcs_Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits
WCS-calibrated image found: wcs_Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits
Checking if the catalog wcs_Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits.cat corresponding to the image wcs_Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits alredy exist and is non-empty...
Catalog wcs_Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits.cat corresponding to the image wcs_Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits
WCS catalog name: wcs_Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits.cat
SExtractor catalog parsing summary: zero_flux=9, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=779, passed=11586
Got 11586 stars (including 10792 good ones) from the SExtractor catalog wcs_Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits.cat
util/solve_plate_with_UCAC5 got 11586 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 927 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: 0.30"
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 927 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.30"
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 927 stars left (next iteration limit 1019)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits -region wcs_Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.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.eB8wwtYERS (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits
WCS_IMAGE_NAME=wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits
WCS-calibrated image found: wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits
Checking if the catalog wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits.cat corresponding to the image wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits.cat corresponding to the image wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits
WCS catalog name: wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=168, passed=3296
Got 3296 stars (including 3126 good ones) from the SExtractor catalog wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits.cat
util/solve_plate_with_UCAC5 got 3296 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.3'
Seting catalog search parameters based on the expected field of view 939.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013046 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010437 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 928 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: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.50"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.50"
Estimated accuracy of the plate solution: 0.50"
Excluding outliers - 928 stars left (next iteration limit 1020)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits -region wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.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.do7kkc4CpN (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits
WCS_IMAGE_NAME=wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits
WCS-calibrated image found: wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits
Checking if the catalog wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits.cat corresponding to the image wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits.cat corresponding to the image wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits
WCS catalog name: wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=164, passed=3238
Got 3238 stars (including 3071 good ones) from the SExtractor catalog wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits.cat
util/solve_plate_with_UCAC5 got 3238 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.3'
Seting catalog search parameters based on the expected field of view 939.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013046 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010437 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 926 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: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 926 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.49"
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 926 stars left (next iteration limit 1018)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits -region wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.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_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits'
Saving fully-calibrated image wcs_Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/wcs_Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits'
Saving fully-calibrated image wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits'
Saving fully-calibrated image wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits'
Preparing the HTML report for the field Peg-09-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20936.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out06131.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 4s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
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Considering the candidate 20936_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558
The candidate 20936_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558 did not pass the final checks
**** FOUND 22:21:58.17 +13:46:38.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.71, MAG_FAINT_SEARCH_LIMIT=11.69)GAIADR2_OUTPUT=# 0.249 2734337263382142080 335.49243255623 +13.77737383667 10.0587 8.6379 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.249#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 06131_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558
Preparing report for the candidate 06131_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 5s
Prepared the HTML report for the field Peg-09-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 ####
22:03:33.93 +14:00:30.7
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/Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits
SExtractor catalog cache: saved Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits.cat to cache
SExtractor catalog cache: saved Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits
Creating symlink local_wcs_cache/wcs_Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits
Creating symlink local_wcs_cache/wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits
Creating symlink local_wcs_cache/wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.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_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits exists and is non-empty
wcs_Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits exists and is non-empty
wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits exists and is non-empty
wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.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 22:13:37.402 +13:59:12.14
Second-epoch image center 22:13:40.188 +13:59:18.21
Angular distance between the image centers 0.01 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 22:13:37.402 +13:59:12.14
Second-epoch image center 22:13:40.124 +13:59:13.72
Angular distance between the image centers 0.01 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 22:13:40.188 +13:59:18.21
Second-epoch second image center 22:13:40.124 +13:59:13.72
Angular distance between the image centers 0.00127 deg.
###################################
ERROR: no shift applied between second-epoch images! The distance between image centers is 0.00127 deg. (min. required shift: 0.00164 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/Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits &> /tmp/tmp.XokeAoq2aA
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits &> /tmp/tmp.fllRv9ELMC
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits &> /tmp/tmp.zDNmJNrIqG
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits &> /tmp/tmp.UeBeM6TXMM
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits
Calibrating the magnitude scale
Found non-empty wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.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_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits and wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.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_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits and wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits.cat
Found non-empty wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits and wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits.cat
The reference image (wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits) and catalog (wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits.cat) found
'wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.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 6908 out of 74327 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.781482
a=0.000000 b=1.000000 c=22.781482
From vast_summary.log: estimated ref. image limiting mag.: -7.38
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.40
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.40
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 14 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits
2.0 pix Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits
2.7 pix fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits
2.8 pix fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits
Limiting magnitude estimates:
15.4 mag. Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits
15.4 mag. Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits
13.5 mag. fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits
13.4 mag. fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits
All-image limiting magnitude estimate: 13.4 (SNR ) 13.0 (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.XokeAoq2aA (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/Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits' -> 'wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits
WCS_IMAGE_NAME=wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits
WCS-calibrated image found: wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits
Checking if the catalog wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits.cat corresponding to the image wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits alredy exist and is non-empty...
Catalog wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits.cat corresponding to the image wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits
WCS catalog name: wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits.cat
SExtractor catalog parsing summary: zero_flux=2, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=4699, passed=74306
Got 74306 stars (including 69479 good ones) from the SExtractor catalog wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits.cat
util/solve_plate_with_UCAC5 got 74306 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 929 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 929 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: 0.32"
Excluding outliers - 929 stars left (next iteration limit 1021)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits -region wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.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.fllRv9ELMC (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/Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits' -> 'wcs_Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits
WCS_IMAGE_NAME=wcs_Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits
WCS-calibrated image found: wcs_Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits
Checking if the catalog wcs_Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits.cat corresponding to the image wcs_Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits alredy exist and is non-empty...
Catalog wcs_Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits.cat corresponding to the image wcs_Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits
WCS catalog name: wcs_Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits.cat
SExtractor catalog parsing summary: zero_flux=7, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=4619, passed=74721
Got 74721 stars (including 69976 good ones) from the SExtractor catalog wcs_Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits.cat
util/solve_plate_with_UCAC5 got 74721 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 927 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 927 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: 0.30"
Excluding outliers - 927 stars left (next iteration limit 1019)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits -region wcs_Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.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.zDNmJNrIqG (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits
WCS_IMAGE_NAME=wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits
WCS-calibrated image found: wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits
Checking if the catalog wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits.cat corresponding to the image wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits.cat corresponding to the image wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits
WCS catalog name: wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=832, passed=21079
Got 21079 stars (including 20223 good ones) from the SExtractor catalog wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits.cat
util/solve_plate_with_UCAC5 got 21079 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.3'
Seting catalog search parameters based on the expected field of view 939.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013046 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010437 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 926 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: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 926 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.49"
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 926 stars left (next iteration limit 1018)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits -region wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.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.UeBeM6TXMM (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits
WCS_IMAGE_NAME=wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits
WCS-calibrated image found: wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits
Checking if the catalog wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits.cat corresponding to the image wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits alredy exist and is non-empty...
Catalog wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits.cat corresponding to the image wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits
WCS catalog name: wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=1, blended=972, passed=20415
Got 20415 stars (including 19414 good ones) from the SExtractor catalog wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits.cat
util/solve_plate_with_UCAC5 got 20415 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 939.3'
Seting catalog search parameters based on the expected field of view 939.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013046 (47.0 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010437 (37.6 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 925 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: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.48"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 925 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.48"
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 925 stars left (next iteration limit 1017)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits -region wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.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_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/wcs_Peg-09-Q2b1x1_2025-12-22_19-50-17_20.00sec_-14.90C_LIGHT_0008.fits
Saving fully-calibrated image wcs_Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/wcs_Peg-09-Q2b1x1_2025-12-22_19-51-14_20.00sec_-15.00C_LIGHT_0009.fits
Saving fully-calibrated image wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-42-38_20.00sec_-14.90C_LIGHT_0557.fits
Saving fully-calibrated image wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-27_CI_Peg-09-Q2b1x1_073341_TTUQ2b1x1_17689_ZBci1jry/wcs_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558.fits
Preparing the HTML report for the field Peg-09-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out90642.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out91247.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out91579.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out92481.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out92788.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out41723.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out69018.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out74017.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 4s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 90642_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558
The candidate 90642_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558 did not pass the final checks
**** FOUND 22:12:14.33 +14:32:15.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.79, MAG_FAINT_SEARCH_LIMIT=12.77)GAIADR2_OUTPUT=# 1.225 2735144128823312768 333.05986568604 +14.53741792218 12.1751 11.7112 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.225#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 90969_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558
The candidate 90969_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558 did not pass the final checks
**** FOUND 22:10:44.20 +11:38:22.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 91012_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558
The candidate 91012_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 91247_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558
The candidate 91247_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558 did not pass the final checks
**** FOUND 22:14:23.08 +17:12:31.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 1.579 1775226840908131968 333.59582931056 +17.20853595225 12.2934 11.8042 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.579#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 91353_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558
The candidate 91353_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 91579_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558
The candidate 91579_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558 did not pass the final checks
**** FOUND 21:55:49.42 +13:48:47.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.52, MAG_FAINT_SEARCH_LIMIT=13.50)GAIADR2_OUTPUT=# 3.621 1768166709242371968 328.95570752971 +13.81223715179 12.6067 12.1625 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.621#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 91675_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558
The candidate 91675_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
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Considering the candidate 91778_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558
The candidate 91778_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558 did not pass the final checks
Rejecting candidate as there is no shift in pixel position (shift 0.0 pix) between the two second-epoch detections and REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES is set to 'yes'
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Considering the candidate 92481_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558
The candidate 92481_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558 did not pass the final checks
**** FOUND 22:12:03.99 +11:44:20.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 2.535 2727621789957696768 333.01594263765 +11.73883330770 13.0938 12.4705 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.535#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 92788_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558
The candidate 92788_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558 did not pass the final checks
**** FOUND 22:12:10.44 +14:33:41.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.88, MAG_FAINT_SEARCH_LIMIT=13.86)GAIADR2_OUTPUT=# 3.553 2735144407996939392 333.04251367848 +14.56119359249 13.1746 12.8741 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.553#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 41723_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558
Preparing report for the candidate 41723_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558
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Considering the candidate 69018_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558
Preparing report for the candidate 69018_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558
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Considering the candidate 74017_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558
Preparing report for the candidate 74017_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558
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Considering the candidate 40193_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558
The candidate 40193_fd_Peg-09-Q2b1x1_2026-03-27_06-43-21_20.00sec_-15.00C_LIGHT_0558 did not pass the final checks