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_215106_TTUQ2b1x1_8226_eplw8rZd
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 202437751581524480,2461129.6180,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 202437751581524480 20260330.1180 13.11CV 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/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:04:57.20 +43:20:02.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_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_21-50-13_20_00sec_-10_00C_LIGHT_0066_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_21-49-15_20_00sec_-10_00C_LIGHT_0065_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_21-50-13_20_00sec_-10_00C_LIGHT_0066_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_21-49-15_20_00sec_-10_00C_LIGHT_0065_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 30.1180* 04 33 44.08 +48 06 54.7 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+480657,2461129.6180,13.01,0.05,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 20260330.1180 13.01CV 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_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:33:44.08 +48:06:54.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_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_21-50-13_20_00sec_-10_00C_LIGHT_0066_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_21-49-15_20_00sec_-10_00C_LIGHT_0065_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_21-50-13_20_00sec_-10_00C_LIGHT_0066_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_21-49-15_20_00sec_-10_00C_LIGHT_0065_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 30.1180 2461129.6180 13.63 05:19:09.31 +48:11:23.2
161.02297 6.16355 galactic Aur Second-epoch detections are separated by 0.1" and 6.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J079.7917+48.1893 | 05:19:09.31 +48:11:23.2 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J079.7917+48.1893,2461129.6180,13.63,0.05,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
ATO J079.7917+48.1893 20260330.1180 13.63CV 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/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:19:09.31 +48:11:23.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_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_21-50-13_20_00sec_-10_00C_LIGHT_0066_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_21-49-15_20_00sec_-10_00C_LIGHT_0065_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_21-50-13_20_00sec_-10_00C_LIGHT_0066_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_21-49-15_20_00sec_-10_00C_LIGHT_0065_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 30.1180* 04 21 35.80 +49 37 14.1 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+493714,2461129.6180,12.14,0.05,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 20260330.1180 12.14CV 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_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:21:35.80 +49:37:14.1 ;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_21-50-13_20_00sec_-10_00C_LIGHT_0066_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_21-49-15_20_00sec_-10_00C_LIGHT_0065_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_21-50-13_20_00sec_-10_00C_LIGHT_0066_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_21-49-15_20_00sec_-10_00C_LIGHT_0065_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: 2461129.61833216 30.03.2026 02:50:13.899 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1
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: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 21673
Objects passed selection criteria: 21548
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: 15292
Average stars matched: 14849.5 (97.1063 %)
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 21:55:00 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: 2461129.61833216 30.03.2026 02:50:13.899 /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 100
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.24
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: 40 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): 176890
Objects passed selection criteria: 176389
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: 128562
Average stars matched: 123776 (96.2767 %)
Memory usage VmPeak: 1942048 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 21:59:33 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_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.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_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.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: 2461129.61765998
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_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits exists and is non-empty
Saving wcs_fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits to local_wcs_cache/
'wcs_fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits' -> 'local_wcs_cache/wcs_fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits'
wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.fits exists and is non-empty
Saving wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.fits to local_wcs_cache/
'wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.fits' -> 'local_wcs_cache/wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.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 04:48:01.972 +45:58:04.67
Angular distance between the image centers 0.03 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 04:48:01.099 +45:59:45.51
Second-epoch image center 04:47:59.232 +45:57:38.88
Angular distance between the image centers 0.04 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 04:48:01.972 +45:58:04.67
Second-epoch second image center 04:47:59.232 +45:57:38.88
Angular distance between the image centers 0.01069 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.qiSaFxa425
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.o562U4Euxl
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_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits &> /tmp/tmp.5f0R0DdHFK
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.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_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.fits &> /tmp/tmp.3IlcZNvLVM
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.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_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits
2.5 pix fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.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_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits
14.0 mag. fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.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.qiSaFxa425 (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_215106_TTUQ2b1x1_8226_eplw8rZd/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.o562U4Euxl (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_215106_TTUQ2b1x1_8226_eplw8rZd/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.5f0R0DdHFK (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_215106_TTUQ2b1x1_8226_eplw8rZd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.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_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits
WCS_IMAGE_NAME=wcs_fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits
WCS-calibrated image found: wcs_fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits
Checking if the catalog wcs_fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits.cat corresponding to the image wcs_fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits.cat corresponding to the image wcs_fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.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_21-49-15_20.00sec_-10.00C_LIGHT_0065.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_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits
WCS catalog name: wcs_fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=530, passed=8408
Got 8408 stars (including 7864 good ones) from the SExtractor catalog wcs_fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits.cat
util/solve_plate_with_UCAC5 got 8408 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: 0.64"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.65"
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: 0.65"
Estimated accuracy of the plate solution: 0.74"
Excluding outliers - 937 stars left (next iteration limit 1030)
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_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.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_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits -region wcs_fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.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.3IlcZNvLVM (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_215106_TTUQ2b1x1_8226_eplw8rZd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.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_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.fits
WCS_IMAGE_NAME=wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.fits
WCS-calibrated image found: wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.fits
Checking if the catalog wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.fits.cat corresponding to the image wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.fits.cat corresponding to the image wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.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_21-50-13_20.00sec_-10.00C_LIGHT_0066.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_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.fits
WCS catalog name: wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=530, passed=8389
Got 8389 stars (including 7852 good ones) from the SExtractor catalog wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.fits.cat
util/solve_plate_with_UCAC5 got 8389 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 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.64"
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 942 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: 0.74"
Excluding outliers - 938 stars left (next iteration limit 1030)
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_21-50-13_20.00sec_-10.00C_LIGHT_0066.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.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_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.fits -region wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.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_215106_TTUQ2b1x1_8226_eplw8rZd/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_215106_TTUQ2b1x1_8226_eplw8rZd/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_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215106_TTUQ2b1x1_8226_eplw8rZd/wcs_fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits'
Saving fully-calibrated image wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215106_TTUQ2b1x1_8226_eplw8rZd/wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.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_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.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_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.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_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits
Creating symlink local_wcs_cache/wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.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_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits exists and is non-empty
wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.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 04:48:01.972 +45:58:04.67
Angular distance between the image centers 0.03 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 04:48:01.099 +45:59:45.51
Second-epoch image center 04:47:59.232 +45:57:38.88
Angular distance between the image centers 0.04 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 04:48:01.972 +45:58:04.67
Second-epoch second image center 04:47:59.232 +45:57:38.88
Angular distance between the image centers 0.01069 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.y8t8ZKMQ2w
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.DhyvoDgvfO
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_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits &> /tmp/tmp.XvGiQc2CL0
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.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_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.fits &> /tmp/tmp.eHxhEXvwDj
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.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 61 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_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits
2.3 pix fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.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
14.0 mag. fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits
14.0 mag. fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.fits
All-image limiting magnitude estimate: 14.0 (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.y8t8ZKMQ2w (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_215106_TTUQ2b1x1_8226_eplw8rZd/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=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.DhyvoDgvfO (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_215106_TTUQ2b1x1_8226_eplw8rZd/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.XvGiQc2CL0 (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_215106_TTUQ2b1x1_8226_eplw8rZd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.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_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits
WCS_IMAGE_NAME=wcs_fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits
WCS-calibrated image found: wcs_fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits
Checking if the catalog wcs_fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits.cat corresponding to the image wcs_fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits.cat corresponding to the image wcs_fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.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_21-49-15_20.00sec_-10.00C_LIGHT_0065.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_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits
WCS catalog name: wcs_fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=2, blended=4379, passed=68066
Got 68066 stars (including 63599 good ones) from the SExtractor catalog wcs_fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits.cat
util/solve_plate_with_UCAC5 got 68066 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 939 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 939 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: 0.69"
Excluding outliers - 933 stars left (next iteration limit 1026)
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_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.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_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits -region wcs_fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.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.eHxhEXvwDj (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_215106_TTUQ2b1x1_8226_eplw8rZd/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-29_CI_Per-03-Q2b1x1_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.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_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.fits
WCS_IMAGE_NAME=wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.fits
WCS-calibrated image found: wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.fits
Checking if the catalog wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.fits.cat corresponding to the image wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.fits alredy exist and is non-empty...
Catalog wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.fits.cat corresponding to the image wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.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_21-50-13_20.00sec_-10.00C_LIGHT_0066.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_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.fits
WCS catalog name: wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=7, blended=4652, passed=68245
Got 68245 stars (including 63510 good ones) from the SExtractor catalog wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.fits.cat
util/solve_plate_with_UCAC5 got 68245 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 940 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: 0.59"
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 940 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 - 934 stars left (next iteration limit 1027)
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_21-50-13_20.00sec_-10.00C_LIGHT_0066.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.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_215106_TTUQ2b1x1_8226_eplw8rZd/fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.fits -region wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.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_215106_TTUQ2b1x1_8226_eplw8rZd/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_215106_TTUQ2b1x1_8226_eplw8rZd/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_21-49-15_20.00sec_-10.00C_LIGHT_0065.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_215106_TTUQ2b1x1_8226_eplw8rZd/wcs_fd_Per-03-Q2b1x1_2026-03-29_21-49-15_20.00sec_-10.00C_LIGHT_0065.fits
Saving fully-calibrated image wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.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_215106_TTUQ2b1x1_8226_eplw8rZd/wcs_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066.fits
Preparing the HTML report for the field Per-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out243593.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out243600.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out243602.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out243607.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out243615.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out243624.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out243633.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out243639.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out244089.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out244115.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out244154.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out244164.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out244178.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out244184.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out244280.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out244305.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out244319.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out244365.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out244398.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out244407.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out244420.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out244433.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out243628.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out244234.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out28761.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out45496.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out58320.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 19s
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: 3s
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Considering the candidate 243593_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 243593_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 04:24:15.20 +42:55:52.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)
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Considering the candidate 243600_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 243600_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 04:20:27.02 +42:30:52.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)
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Considering the candidate 243602_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 243602_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 04:32:16.49 +43:55:57.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)
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Considering the candidate 243604_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 243604_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 05:00:23.75 +45:10:25.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 243607_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 243607_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 05:04:10.92 +42:19:49.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 1.547 202124773023245952 076.04525213416 +42.33088857937 13.6529 13.2679 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.547#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 243615_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 243615_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 05:03:09.54 +41:50:02.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 0.319 201727437009012480 075.78963789800 +41.83414065193 13.2699 13.0057 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.319#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 243622_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 243622_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 04:36:23.36 +43:12:05.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 243624_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 243624_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 05:19:47.30 +42:06:48.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 2.092 195131810349367808 079.94705312757 +42.11289156742 13.1326 12.2521 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.092#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_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 243628_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 04:50:51.90 +42:58:45.4 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)
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Considering the candidate 243630_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 243630_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 04:51:55.90 +42:03:21.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 243631_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 243631_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 05:21:00.16 +43:23:56.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 243633_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 243633_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 04:12:33.39 +46:32:47.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.74, MAG_FAINT_SEARCH_LIMIT=13.72)
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Considering the candidate 243639_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 243639_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 05:05:27.92 +42:38:02.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 1.252 202182085066634240 076.36668407352 +42.63414999222 13.2267 12.6895 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.252#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 243644_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 243644_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 04:56:51.06 +42:50:53.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 243650_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 243650_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
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Considering the candidate 243652_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 243652_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 04:30:26.74 +41:49:50.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244045_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 244045_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 04:52:57.44 +42:34:50.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 244061_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 244061_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 04:37:02.52 +42:06:18.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244089_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 244089_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 05:01:35.00 +48:48:43.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.80, MAG_FAINT_SEARCH_LIMIT=13.78)GAIADR2_OUTPUT=# 2.257 255527017693756928 075.39666636379 +48.81175191378 12.2804 11.1919 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.257#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 244093_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 244093_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 05:18:23.57 +48:55:05.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244115_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 244115_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 04:53:14.36 +43:50:08.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 1.540 205324588079752576 073.30934144699 +43.83593363555 13.1981 12.8169 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.540#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 244123_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 244123_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 05:12:14.30 +45:35:50.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244139_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 244139_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 04:47:24.64 +46:00:22.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244154_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 244154_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 05:22:39.83 +47:54:50.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 0.080 212586660519063680 080.66597215012 +47.91400751652 13.0455 12.2084 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.080#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 244164_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 244164_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 04:48:56.36 +43:15:34.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 2.885 204530809401845120 072.23493970524 +43.25881358801 12.7969 11.9198 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.885#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 244166_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 244166_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 04:36:40.78 +45:00:59.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244178_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 244178_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 04:46:21.10 +42:21:56.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.98, MAG_FAINT_SEARCH_LIMIT=13.96)GAIADR2_OUTPUT=# 2.146 203722152963258240 071.58711460818 +42.36565787802 13.1761 12.4277 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.146#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 244179_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 244179_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 04:49:57.24 +41:43:16.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244184_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 244184_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 04:46:53.69 +43:00:39.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 2.031 204506040331096832 071.72294954622 +43.01107379155 13.1789 12.6150 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.031#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 244197_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 244197_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 04:24:24.56 +41:42:27.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244199_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 244199_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 05:10:21.98 +41:54:22.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244222_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 244222_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 04:51:41.87 +42:03:21.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244234_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
Preparing report for the candidate 244234_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
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Considering the candidate 244276_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 244276_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 04:17:16.01 +46:11:56.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244280_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 244280_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 05:17:20.76 +45:22:42.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 5.109 208690330609106176 079.33734636330 +45.37718365468 13.0811 12.2318 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.109#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 244288_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 244288_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 04:55:24.08 +43:25:00.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244305_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 244305_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 05:07:03.47 +45:01:50.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 4.754 205709249647703296 076.76506135839 +45.02933350376 13.2262 12.6198 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.754#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 244307_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 244307_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 04:45:19.27 +47:28:46.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244315_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 244315_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 05:17:56.76 +46:08:23.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244319_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 244319_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 05:15:48.26 +47:08:42.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 1.269 212085489375748608 078.95131909660 +47.14479734797 13.2771 12.4544 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.269#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 244321_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 244321_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 04:35:36.59 +45:11:50.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244365_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 244365_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 04:55:50.66 +43:08:30.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 2.281 205048030842622464 073.96069740378 +43.14123808740 13.1424 12.2288 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.281#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 244366_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 244366_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 05:10:48.19 +46:56:05.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 244398_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 244398_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 04:46:54.93 +43:00:57.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)
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Considering the candidate 244407_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 244407_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 05:02:07.04 +44:00:58.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)GAIADR2_OUTPUT=# 1.423 205550782533605376 075.52891398178 +44.01602208641 13.7833 13.1996 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.423#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 244420_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 244420_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 04:40:04.65 +43:17:02.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 1.004 204709892361784192 070.01945000406 +43.28416243414 13.2881 12.3080 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.004#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 244424_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 244424_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 05:01:55.76 +42:43:43.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244433_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 244433_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 04:48:15.57 +42:48:53.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 4.056 203746827551228160 072.06609317885 +42.81546411893 13.7163 13.1568 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.056#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 244436_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 244436_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 04:46:35.13 +42:20:25.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244441_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 244441_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 04:49:23.21 +44:13:16.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244462_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 244462_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 04:28:17.75 +44:43:09.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244467_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 244467_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 04:48:26.14 +43:18:58.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244473_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 244473_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 05:04:16.17 +45:48:23.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 244504_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 244504_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 04:45:39.23 +48:10:29.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 172015_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 172015_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 04:27:32.48 +41:47:05.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 18699_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 18699_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 04:31:05.34 +50:10:25.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75612_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 75612_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks
**** FOUND 04:34:13.02 +47:15:36.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 58320_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
Preparing report for the candidate 58320_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
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Considering the candidate 56818_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066
The candidate 56818_fd_Per-03-Q2b1x1_2026-03-29_21-50-13_20.00sec_-10.00C_LIGHT_0066 did not pass the final checks