This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ
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!
TCP 2026 03 30.1190* 04 25 56.56 +49 53 23.0 12.7 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J042556.16+495325.8,2461129.6190,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J042556.16+495325.8 20260330.1190 12.74CV 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/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:25:56.56 +49:53:23.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20_00sec_-10_00C_LIGHT_0068_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20_00sec_-10_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20_00sec_-10_00C_LIGHT_0068_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20_00sec_-10_00C_LIGHT_0067_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 30.1190* 04 33 44.02 +48 06 53.4 13.0 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0433439+480657,2461129.6190,12.99,0.05,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
NSVS J0433439+480657 20260330.1190 12.99CV 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/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:33:44.02 +48:06:53.4 ;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_Per-03-Q2b1x1_2026-02-11_20-38-38_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20_00sec_-10_00C_LIGHT_0068_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20_00sec_-10_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20_00sec_-10_00C_LIGHT_0068_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20_00sec_-10_00C_LIGHT_0067_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J050411.82+463631.1,2461129.6190,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J050411.82+463631.1 20260330.1190 13.03CV 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/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:04:11.67 +46:36:31.5 ;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_Per-03-Q2b1x1_2026-02-11_20-38-38_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20_00sec_-10_00C_LIGHT_0068_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20_00sec_-10_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20_00sec_-10_00C_LIGHT_0068_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20_00sec_-10_00C_LIGHT_0067_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 30.1190* 04 21 35.90 +49 37 13.0 12.1 U Per 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0421353+493714,2461129.6190,12.09,0.05,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
NSVS J0421353+493714 20260330.1190 12.09CV 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/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:21:35.90 +49:37:13.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20_00sec_-10_00C_LIGHT_0068_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20_00sec_-10_00C_LIGHT_0067_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20_00sec_-10_00C_LIGHT_0068_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png resample_wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20_00sec_-10_00C_LIGHT_0067_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: 2461083.61028419 12.02.2026 02:38:38.554 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
First image: 2461083.61028419 12.02.2026 02:38:38.554 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
Last image: 2461129.61935075 30.03.2026 02:51:41.905 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.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.: -7.57
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): 21677
Objects passed selection criteria: 21550
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 15332.5
Average stars matched: 14889.8 (97.1123 %)
Memory usage VmPeak: 127336 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 Sun Mar 29 21:59:00 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: 2461083.61028419 12.02.2026 02:38:38.554 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
First image: 2461083.61028419 12.02.2026 02:38:38.554 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
Last image: 2461129.61935075 30.03.2026 02:51:41.905 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 103
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.24
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: 45 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): 176919
Objects passed selection criteria: 176419
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 129039
Average stars matched: 124276 (96.3085 %)
Memory usage VmPeak: 1942044 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 Sun Mar 29 22:03:47 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/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits
SExtractor catalog cache: saved Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits.cat to cache
SExtractor catalog cache: saved Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.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/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.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: 2461129.61869503
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits exists and is non-empty
Saving wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits to local_wcs_cache/
'wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits' -> 'local_wcs_cache/wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits'
wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits exists and is non-empty
Saving wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits to local_wcs_cache/
'wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits' -> 'local_wcs_cache/wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits'
wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits exists and is non-empty
Saving wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits to local_wcs_cache/
'wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits' -> 'local_wcs_cache/wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits'
wcs_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits exists and is non-empty
Saving wcs_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits to local_wcs_cache/
'wcs_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits' -> 'local_wcs_cache/wcs_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.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 04:48:01.099 +45:59:45.51
Second-epoch image center 04:47:59.220 +45:57:40.02
Angular distance between the image centers 0.04 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 04:48:01.099 +45:59:45.51
Second-epoch image center 04:48:01.689 +45:58:11.15
Angular distance between the image centers 0.03 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 04:47:59.220 +45:57:40.02
Second-epoch second image center 04:48:01.689 +45:58:11.15
Angular distance between the image centers 0.01122 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/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits &> /tmp/tmp.r3Xbm6XRPV
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits &> /tmp/tmp.aRdT4czJoG
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits &> /tmp/tmp.2M0MU77zMP
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits &> /tmp/tmp.D9GI4N94t6
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits
Calibrating the magnitude scale
Found non-empty wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.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_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits and wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.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_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits and wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits.cat
Found non-empty wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits and wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits.cat
The reference image (wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits) and catalog (wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits.cat) found
'wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.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 9281 out of 27125 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.966720
a=0.000000 b=1.000000 c=22.966720
From vast_summary.log: estimated ref. image limiting mag.: -7.57
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 0 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
2.0 pix Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
2.5 pix fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits
2.4 pix fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits
Limiting magnitude estimates:
15.4 mag. Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
15.4 mag. Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
14.0 mag. fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits
14.0 mag. fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 11.2 (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.r3Xbm6XRPV (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/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.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_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits' -> 'wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
WCS_IMAGE_NAME=wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
WCS-calibrated image found: wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
Checking if the catalog wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits.cat corresponding to the image wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits alredy exist and is non-empty...
Catalog wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits.cat corresponding to the image wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
WCS catalog name: wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2857, passed=27125
Got 27125 stars (including 24239 good ones) from the SExtractor catalog wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits.cat
util/solve_plate_with_UCAC5 got 27125 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.40"
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 961 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.40"
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits -region wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.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.aRdT4czJoG (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/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.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_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits' -> 'wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
WCS_IMAGE_NAME=wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
WCS-calibrated image found: wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
Checking if the catalog wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits.cat corresponding to the image wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits alredy exist and is non-empty...
Catalog wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits.cat corresponding to the image wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
WCS catalog name: wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2852, passed=27075
Got 27075 stars (including 24193 good ones) from the SExtractor catalog wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits.cat
util/solve_plate_with_UCAC5 got 27075 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.40"
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 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.40"
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 955 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits -region wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.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.2M0MU77zMP (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_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.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_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits
WCS_IMAGE_NAME=wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits
WCS-calibrated image found: wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits
Checking if the catalog wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits.cat corresponding to the image wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits.cat corresponding to the image wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits
WCS catalog name: wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=540, passed=8454
Got 8454 stars (including 7909 good ones) from the SExtractor catalog wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits.cat
util/solve_plate_with_UCAC5 got 8454 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 944 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: 0.66"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.64"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.65"
Estimated accuracy of the plate solution: 0.76"
Excluding outliers - 940 stars left (next iteration limit 1032)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits -region wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.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.D9GI4N94t6 (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_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.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_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits
WCS_IMAGE_NAME=wcs_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits
WCS-calibrated image found: wcs_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits
Checking if the catalog wcs_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits.cat corresponding to the image wcs_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits.cat corresponding to the image wcs_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits
WCS catalog name: wcs_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=564, passed=8518
Got 8518 stars (including 7940 good ones) from the SExtractor catalog wcs_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits.cat
util/solve_plate_with_UCAC5 got 8518 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.63"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.63"
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 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.64"
Estimated accuracy of the plate solution: 0.72"
Excluding outliers - 939 stars left (next iteration limit 1031)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits -region wcs_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.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_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits'
Saving fully-calibrated image wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits'
Saving fully-calibrated image wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits'
Saving fully-calibrated image wcs_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/wcs_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits'
Preparing the HTML report for the field Per-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
No candidates found here
Prepared the HTML report for the field Per-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits
SExtractor catalog cache: saved Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits.cat to cache
SExtractor catalog cache: saved Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
Creating symlink local_wcs_cache/wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
Creating symlink local_wcs_cache/wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits
Creating symlink local_wcs_cache/wcs_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.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_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits exists and is non-empty
wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits exists and is non-empty
wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits exists and is non-empty
wcs_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.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 04:48:01.099 +45:59:45.51
Second-epoch image center 04:47:59.220 +45:57:40.02
Angular distance between the image centers 0.04 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 04:48:01.099 +45:59:45.51
Second-epoch image center 04:48:01.689 +45:58:11.15
Angular distance between the image centers 0.03 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 04:47:59.220 +45:57:40.02
Second-epoch second image center 04:48:01.689 +45:58:11.15
Angular distance between the image centers 0.01122 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/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits &> /tmp/tmp.nvUl9Vt6fn
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits &> /tmp/tmp.REnEGAl9cx
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits &> /tmp/tmp.aGj6IWFIKg
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits &> /tmp/tmp.EzHi6iTrSd
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits
Calibrating the magnitude scale
Found non-empty wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.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_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits and wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.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_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits and wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits.cat
Found non-empty wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits and wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits.cat
The reference image (wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits) and catalog (wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits.cat) found
'wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.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 9346 out of 215662 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.835556
a=0.000000 b=1.000000 c=22.835556
From vast_summary.log: estimated ref. image limiting mag.: -7.24
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.60
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.60
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 57 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.8 pix Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
1.8 pix Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
2.3 pix fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits
2.3 pix fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits
Limiting magnitude estimates:
15.6 mag. Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
15.6 mag. Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
14.1 mag. fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits
14.1 mag. fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 13.5 (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.nvUl9Vt6fn (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/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.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_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/util/wcs_image_calibration.sh: line 129: echo: write error: Broken pipe
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits' -> 'wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
WCS_IMAGE_NAME=wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
WCS-calibrated image found: wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
Checking if the catalog wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits.cat corresponding to the image wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits alredy exist and is non-empty...
Catalog wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits.cat corresponding to the image wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
WCS catalog name: wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=60, blended=30564, passed=215602
Got 215602 stars (including 184715 good ones) from the SExtractor catalog wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits.cat
util/solve_plate_with_UCAC5 got 215602 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.40"
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits -region wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.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.REnEGAl9cx (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/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.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_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits' -> 'wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
WCS_IMAGE_NAME=wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
WCS-calibrated image found: wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
Checking if the catalog wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits.cat corresponding to the image wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits alredy exist and is non-empty...
Catalog wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits.cat corresponding to the image wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
WCS catalog name: wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=62, blended=30755, passed=215764
Got 215764 stars (including 184684 good ones) from the SExtractor catalog wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits.cat
util/solve_plate_with_UCAC5 got 215764 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.41"
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 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.41"
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 962 stars left (next iteration limit 1058)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits -region wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.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.aGj6IWFIKg (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_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.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_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits
WCS_IMAGE_NAME=wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits
WCS-calibrated image found: wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits
Checking if the catalog wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits.cat corresponding to the image wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits.cat corresponding to the image wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits
WCS catalog name: wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=4529, passed=68411
Got 68411 stars (including 63802 good ones) from the SExtractor catalog wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits.cat
util/solve_plate_with_UCAC5 got 68411 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.65"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.58"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 945 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.59"
Estimated accuracy of the plate solution: 0.69"
Excluding outliers - 939 stars left (next iteration limit 1031)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits -region wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.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.EzHi6iTrSd (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_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.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_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits
WCS_IMAGE_NAME=wcs_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits
WCS-calibrated image found: wcs_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits
Checking if the catalog wcs_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits.cat corresponding to the image wcs_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits.cat corresponding to the image wcs_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits
WCS catalog name: wcs_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=5, blended=4814, passed=69926
Got 69926 stars (including 65017 good ones) from the SExtractor catalog wcs_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits.cat
util/solve_plate_with_UCAC5 got 69926 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010411 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 944 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: 0.64"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.60"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.60"
Estimated accuracy of the plate solution: 0.73"
Excluding outliers - 940 stars left (next iteration limit 1032)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits -region wcs_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.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_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.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_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/wcs_Per-03-Q2b1x1_2026-02-11_20-38-38_20.00sec_-15.00C_LIGHT_0043.fits
Saving fully-calibrated image wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.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_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/wcs_Per-03-Q2b1x1_2026-02-11_20-39-32_20.00sec_-14.90C_LIGHT_0044.fits
Saving fully-calibrated image wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.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_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-45_20.00sec_-10.00C_LIGHT_0067.fits
Saving fully-calibrated image wcs_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.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_2026-03-29_CI_Per-03-Q2b1x1_215503_TTUQ2b1x1_1158_HlaegesQ/wcs_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068.fits
Preparing the HTML report for the field Per-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out243611.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out243613.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out243614.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out243617.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out243622.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out243626.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out243636.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out243849.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out244103.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out244170.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out244191.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out244216.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out244224.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out244227.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out244230.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out244259.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out244298.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out244390.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out244462.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out244484.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out243637.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out23829.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28761.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out58320.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out82979.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 13s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 243611_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
The candidate 243611_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068 did not pass the final checks
**** FOUND 05:19:47.34 +42:06:49.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 3.135 195131810349367808 079.94705312757 +42.11289156742 13.1326 12.2521 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.135#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 243613_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
The candidate 243613_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068 did not pass the final checks
**** FOUND 04:52:24.05 +41:46:36.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)
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Considering the candidate 243614_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
The candidate 243614_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068 did not pass the final checks
**** FOUND 05:03:28.78 +49:06:43.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 3.162 255538704301505024 075.86945546610 +49.11285262281 13.8023 13.1609 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.162#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 243617_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
The candidate 243617_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068 did not pass the final checks
**** FOUND 04:50:35.25 +43:33:03.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 0.925 206041645758877568 072.64711810625 +43.55124268459 13.1924 12.8684 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.925#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 243620_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
The candidate 243620_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068 did not pass the final checks
**** FOUND 04:36:23.29 +43:12:05.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 243622_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
The candidate 243622_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068 did not pass the final checks
**** FOUND 04:17:27.61 +44:34:11.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 1.352 232618250549684224 064.36546426509 +44.56958105626 13.2831 12.8540 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.352#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 243625_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
The candidate 243625_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068 did not pass the final checks
**** FOUND 05:21:00.25 +43:23:56.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 243626_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
The candidate 243626_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068 did not pass the final checks
**** FOUND 05:07:20.49 +42:24:09.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 1.908 201386519684866560 076.83608585316 +42.40245352687 13.0889 12.6230 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.908#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 243628_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
The candidate 243628_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068 did not pass the final checks
**** FOUND 04:47:05.66 +49:02:49.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 243633_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
The candidate 243633_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 243635_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
The candidate 243635_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068 did not pass the final checks
**** FOUND 04:30:18.91 +45:56:10.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 243636_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
The candidate 243636_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068 did not pass the final checks
**** FOUND 04:23:52.99 +49:48:40.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 3.731 270463062821083008 065.97146788258 +49.81221794097 12.8554 12.1297 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.731#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 243637_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
The candidate 243637_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068 did not pass the final checks
**** FOUND 04:50:51.92 +42:58:45.4 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)
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Considering the candidate 243638_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
The candidate 243638_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068 did not pass the final checks
**** FOUND 04:56:51.06 +42:50:52.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 243645_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
The candidate 243645_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068 did not pass the final checks
**** FOUND 05:03:55.49 +42:53:59.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 243646_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
The candidate 243646_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068 did not pass the final checks
**** FOUND 04:30:26.71 +41:49:49.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 243849_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
The candidate 243849_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068 did not pass the final checks
**** FOUND 04:55:46.93 +43:10:22.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 0.885 205049027275022720 073.94527086713 +43.17274235451 11.8818 11.1032 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.885#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 244014_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
The candidate 244014_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068 did not pass the final checks
**** FOUND 04:37:02.52 +42:06:19.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244019_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
The candidate 244019_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068 did not pass the final checks
**** FOUND 04:52:57.49 +42:34:50.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 244078_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
The candidate 244078_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068 did not pass the final checks
**** FOUND 05:18:23.76 +48:55:05.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244096_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
The candidate 244096_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068 did not pass the final checks
**** FOUND 04:47:24.60 +46:00:22.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244103_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
The candidate 244103_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068 did not pass the final checks
**** FOUND 05:01:34.97 +48:48:43.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 2.718 255527017693756928 075.39666636379 +48.81175191378 12.2804 11.1919 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.718#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 244116_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
The candidate 244116_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068 did not pass the final checks
**** FOUND 05:12:14.26 +45:35:50.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244128_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
The candidate 244128_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068 did not pass the final checks
**** FOUND 04:49:57.27 +41:43:16.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244140_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
The candidate 244140_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068 did not pass the final checks
**** FOUND 04:51:41.71 +42:03:20.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244149_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
The candidate 244149_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068 did not pass the final checks
**** FOUND 04:36:40.77 +45:00:58.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244170_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
The candidate 244170_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068 did not pass the final checks
**** FOUND 04:46:21.07 +42:21:54.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 2.668 203722152963258240 071.58711460818 +42.36565787802 13.1761 12.4277 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.668#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 244178_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
The candidate 244178_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068 did not pass the final checks
**** FOUND 04:24:24.60 +41:42:27.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244191_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
The candidate 244191_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068 did not pass the final checks
**** FOUND 05:04:57.08 +43:20:05.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.13, MAG_FAINT_SEARCH_LIMIT=14.11)GAIADR2_OUTPUT=# 4.004 202437755878699264 076.23647985353 +43.33537866064 13.6822 13.0506 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.004#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 244214_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
The candidate 244214_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068 did not pass the final checks
**** FOUND 04:35:36.61 +45:11:50.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244216_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
The candidate 244216_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068 did not pass the final checks
**** FOUND 04:56:55.88 +43:07:58.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)GAIADR2_OUTPUT=# 3.009 205126641624574464 074.23303912962 +43.13365562550 13.1035 12.2198 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.009#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 244224_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
The candidate 244224_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068 did not pass the final checks
**** FOUND 04:46:53.82 +43:00:39.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 3.424 204506040331096832 071.72294954622 +43.01107379155 13.1789 12.6150 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.424#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 244227_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
The candidate 244227_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068 did not pass the final checks
**** FOUND 04:48:56.29 +43:15:33.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 2.319 204530809401845120 072.23493970524 +43.25881358801 12.7969 11.9198 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.319#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 244230_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
The candidate 244230_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068 did not pass the final checks
**** FOUND 05:10:58.46 +43:36:17.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 1.190 202350585223155456 077.74333048732 +43.60461366733 13.5849 13.1844 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.190#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 244259_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
The candidate 244259_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068 did not pass the final checks
**** FOUND 05:17:20.74 +45:22:42.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.25, MAG_FAINT_SEARCH_LIMIT=14.23)GAIADR2_OUTPUT=# 5.201 208690330609106176 079.33734636330 +45.37718365468 13.0811 12.2318 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.201#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 244268_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
The candidate 244268_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068 did not pass the final checks
**** FOUND 04:45:19.24 +47:28:47.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244291_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
The candidate 244291_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068 did not pass the final checks
**** FOUND 04:55:24.20 +43:25:00.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244298_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
The candidate 244298_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068 did not pass the final checks
**** FOUND 04:59:49.64 +41:52:44.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 2.888 201774196315797120 074.95758733181 +41.87845476207 13.4597 13.0455 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.888#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 244315_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
The candidate 244315_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068 did not pass the final checks
**** FOUND 05:17:56.65 +46:08:24.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244322_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
The candidate 244322_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068 did not pass the final checks
**** FOUND 04:58:04.30 +43:14:05.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244330_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
The candidate 244330_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068 did not pass the final checks
**** FOUND 04:58:37.79 +44:25:40.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244349_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
The candidate 244349_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068 did not pass the final checks
**** FOUND 05:10:22.00 +41:54:25.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244372_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
The candidate 244372_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068 did not pass the final checks
**** FOUND 04:48:26.09 +43:18:58.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244390_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
The candidate 244390_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068 did not pass the final checks
**** FOUND 05:02:07.07 +44:00:58.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 1.445 205550782533605376 075.52891398178 +44.01602208641 13.7833 13.1996 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.445#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 244418_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
The candidate 244418_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068 did not pass the final checks
**** FOUND 04:27:48.08 +46:15:03.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244451_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
The candidate 244451_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068 did not pass the final checks
**** FOUND 04:49:23.25 +44:13:17.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244462_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
The candidate 244462_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068 did not pass the final checks
**** FOUND 05:08:58.50 +44:38:36.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 0.482 205630084810885632 077.24385893491 +44.64363678493 13.4996 12.6086 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.482#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 244474_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
The candidate 244474_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068 did not pass the final checks
**** FOUND 04:46:20.11 +43:34:19.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244484_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
The candidate 244484_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068 did not pass the final checks
**** FOUND 05:08:50.95 +42:33:34.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 0.850 201487915271599488 077.21256999242 +42.55957734280 13.8618 13.5147 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.850#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 172015_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
The candidate 172015_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068 did not pass the final checks
**** FOUND 04:27:32.53 +41:47:04.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 18699_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
The candidate 18699_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068 did not pass the final checks
**** FOUND 04:31:05.35 +50:10:25.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 23829_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
Preparing report for the candidate 23829_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
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Considering the candidate 75612_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
The candidate 75612_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068 did not pass the final checks
**** FOUND 04:34:13.02 +47:15:35.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58320_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
Preparing report for the candidate 58320_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
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Considering the candidate 82979_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
Preparing report for the candidate 82979_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
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Considering the candidate 56818_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068
The candidate 56818_fd_Per-03-Q2b1x1_2026-03-29_21-51-41_20.00sec_-10.00C_LIGHT_0068 did not pass the final checks